text: A new top-level full-sized model was introduced at mid-year 1959, the Ford Galaxie. The 1959 Galaxie displayed both "Fairlane 500" and "Galaxie" badging.

text: A new top-level full-sized model was introduced at mid-year 1959, the

entity_name: Ford Galaxie

text: Ford Galaxie

text: . The 1959 Galaxie displayed both "Fairlane 500" and "Galaxie" badging.

method: ICT-DRMMTKS

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answers: Galaxie

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answers: galaxie

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answers: Galaxie

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answers: Galaxie

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answers: Galaxie

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answers: Our solar system is slowly spinning around our galaxy.

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answers: Galaxie

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answers: Galaxie

text: ESO 137-001 is a barred spiral galaxy located in the cluster known as Abell 3627 (Norma Cluster). As the galaxy moves to the center of the cluster, it is stripped by hot gas thus creating a 260,000 light-year long tail. There is evidence of star formation in the tails. The galaxy was discovered by Dr. Ming Sun in 2005.

text: ESO 137-001 is a

entity_name: Barred spiral galaxy

text: barred spiral galaxy

text: located in the cluster known as

entity_name: Norma Cluster

text: Abell 3627

text: (Norma Cluster). As the galaxy moves to the center of the cluster, it is stripped by hot gas thus creating a 260,000

entity_name: Light-year

text: light-year

text: long tail. There is evidence of star formation in the tails. The galaxy was discovered by Dr. Ming Sun in 2005.

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answers: NDQ_002600

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answers: a 260,000 light-year long tail

answers: NDQ_002602

answers: barred spiral

answers: NDQ_002603

answers: hot gas

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answers: hot gas

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answers: ESO 137-001

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answers: barred

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answers: The galaxy moves to the center of the cluster

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answers: Abell 3627

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answers: ESO 137-001

answers: NDQ_002632

answers: larger galaxies

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answers: Norma Cluster

answers: NDQ_002635

answers: As the galaxy moves to the center of the cluster

answers: NDQ_002636

answers: The galaxy was discovered

text: Groups and clusters of galaxies have a wider range of velocity dispersions than smaller objects. For example, our own poor group, the  Local Group, has a σ = 61±8 km/s. But rich clusters of galaxies, such as the Coma Cluster, have a σ ≈ 1,000 km/s. The dwarf elliptical galaxies in Coma have their own, internal, velocity dispersion for their stars, which is a σ ≲ 80 km/s, typically. Normal elliptical galaxies, by comparison, have an average σ ≈ 200 km/s.

text: Groups and clusters of galaxies have a wider range of velocity dispersions than smaller objects. For example, our own

entity_name: Abell catalogue

entity_section: Richness

text: poor group

text: , the

entity_name: Local Group

text: Local Group

text: , has a σ = 61±8 km/s. But rich clusters of galaxies, such as the

entity_name: Coma Cluster

text: Coma Cluster

text: , have a σ ≈ 1,000 km/s. The

entity_name: Dwarf elliptical galaxy

text: dwarf elliptical galaxies

text: in Coma have their own, internal, velocity dispersion for their stars, which is a σ ≲ 80 km/s, typically. Normal

entity_name: Elliptical galaxy

text: elliptical galaxies

text: , by comparison, have an average σ ≈ 200 km/s.

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text: The organization of structure arguably begins at the stellar level, though most cosmologists rarely address astrophysics on that scale. Stars are organized into galaxies, which in turn form galaxy groups, galaxy clusters, superclusters, sheets, walls and filaments, which are separated by immense voids, creating a vast foam-like structure sometimes called the "cosmic web". Prior to 1989, it was commonly assumed that virialized galaxy clusters were the largest structures in existence, and that they were distributed more or less uniformly throughout the Universe in every direction. However, since the early 1980s, more and more structures have been discovered. In 1983, Adrian Webster identified the Webster LQG, a large quasar group consisting of 5 quasars. The discovery was the first identification of a large-scale structure, and has expanded the information about the known grouping of matter in the Universe. In 1987, Robert Brent Tully identified the Pisces–Cetus Supercluster Complex, the galaxy filament in which the Milky Way resides. It is about 1 billion light years across. That same year, an unusually large region with no galaxies has been discovered, the Giant Void, which measures 1.3 billion light years across. Based on redshift survey data, in 1989 Margaret Geller and John Huchra discovered the "Great Wall", a sheet of galaxies more than 500 million light-years long and 200 million wide, but only 15 million light-years thick. The existence of this structure escaped notice for so long because it requires locating the position of galaxies in three dimensions, which involves combining location information about the galaxies with distance information from redshifts.Two years later, astronomers Roger G. Clowes and Luis E. Campusano discovered the Clowes–Campusano LQG, a large quasar group measuring two billion light years at its widest point, and was the largest known structure in the Universe at the time of its announcement. In April 2003, another large-scale structure was discovered, the Sloan Great Wall. In August 2007, a possible supervoid was detected in the constellation Eridanus. It coincides with the 'CMB cold spot', a cold region in the microwave sky that is highly improbable under the currently favored cosmological model. This supervoid could cause the cold spot, but to do so it would have to be improbably big, possibly a billion light-years across, almost as big as the Giant Void mentioned above.

text: The organization of structure arguably begins at the stellar level, though most cosmologists rarely address

entity_name: Astrophysics

text: astrophysics

text: on that scale.

entity_name: Star

text: Star

text: s are organized into

entity_name: Galaxy

text: galaxies

text: , which in turn form

entity_name: Galaxy group

text: galaxy group

text: s,

entity_name: Galaxy cluster

text: galaxy cluster

text: s,

entity_name: Supercluster

text: supercluster

text: s, sheets,

entity_name: Galaxy filament

text: walls and filaments

text: , which are separated by immense

entity_name: Void (astronomy)

text: voids

text: , creating a vast foam-like structure sometimes called the "cosmic web". Prior to 1989, it was commonly assumed that

entity_name: Virial theorem

text: virialized

text: galaxy clusters were the largest structures in existence, and that they were distributed more or less uniformly throughout the Universe in every direction. However, since the early 1980s, more and more structures have been discovered. In 1983, Adrian Webster identified the Webster LQG, a

entity_name: Large quasar group

text: large quasar group

text: consisting of 5 quasars. The discovery was the first identification of a large-scale structure, and has expanded the information about the known grouping of matter in the Universe. In 1987, Robert Brent Tully identified the

entity_name: Pisces–Cetus Supercluster Complex

text: Pisces–Cetus Supercluster Complex

text: , the galaxy filament in which the Milky Way resides. It is about 1 billion light years across. That same year, an unusually large region with no galaxies has been discovered, the

entity_name: Giant Void

text: Giant Void

text: , which measures 1.3 billion light years across. Based on

entity_name: Redshift survey

text: redshift survey

text: data, in 1989

entity_name: Margaret Geller

text: Margaret Geller

text: and

entity_name: John Huchra

text: John Huchra

text: discovered the "

entity_name: CfA2 Great Wall

text: Great Wall

text: ", a sheet of galaxies more than 500 million

text: light-year

text: s long and 200 million wide, but only 15 million light-years thick. The existence of this structure escaped notice for so long because it requires locating the position of galaxies in three dimensions, which involves combining location information about the galaxies with distance information from

entity_name: Redshift

text: redshift

text: s.Two years later, astronomers Roger G. Clowes and Luis E. Campusano discovered the

entity_name: Clowes–Campusano LQG

text: Clowes–Campusano LQG

text: , a

text: large quasar group

text: measuring two billion light years at its widest point, and was the largest known structure in the Universe at the time of its announcement. In April 2003, another large-scale structure was discovered, the

entity_name: Sloan Great Wall

text: Sloan Great Wall

text: . In August 2007, a possible supervoid was detected in the constellation

entity_name: Eridanus (constellation)

text: Eridanus

text: . It coincides with the '

entity_name: CMB cold spot

text: CMB cold spot

text: ', a cold region in the microwave sky that is highly improbable under the currently favored cosmological model. This supervoid could cause the cold spot, but to do so it would have to be improbably big, possibly a billion light-years across, almost as big as the Giant Void mentioned above.

method: UNH-ecn

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text: There are two main shape groups: "round pads" and long narrow pads called "bar pads". Pads are also made in other shapes, called "loaf pads". Within each group there are three size categories: small, medium, and large size pads. It is also possible to engineer custom-shaped pads to meet special application requirements.

text: There are two main shape groups: "round pads" and long narrow pads called "bar pads". Pads are also made in other shapes, called "loaf pads". Within each group there are three size categories: small, medium, and large size pads. It is also possible to engineer custom-shaped pads to meet special application requirements.

method: dangnt-nlp

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text: In weak gravitational lensing, the Jacobian is mapped out by observing the effect of the shear on the ellipticities of background galaxies.  This effect is purely statistical; the shape of any galaxy will be dominated by its random, unlensed shape, but lensing will produce a spatially coherent distortion of these shapes.

text: In

entity_name: Weak gravitational lensing

text: weak gravitational lensing

text: , the

entity_name: Gravitational lensing formalism

entity_section: Lensing Jacobian

text: Jacobian

text: is mapped out by observing the effect of the shear on the ellipticities of background galaxies.  This effect is purely statistical; the shape of any galaxy will be dominated by its random, unlensed shape, but lensing will produce a spatially coherent distortion of these shapes.

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answers: The shape of any galaxy will be dominated by its random, unlensed shape

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text: The Milky Way galaxy is part of a group of galaxies called the Local Group.

text: The

entity_name: Milky Way

text: Milky Way

text: galaxy is part of a group of galaxies called the

text: Local Group

method: UNH-tfidf-stem

method: UNH-tfidf-ptsim

method: UNH-tfidf-lem

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text: The city was initially designed in the shape of the Buddhist Dharma-Chakra (Wheel of Righteousness). The four thurs or mounds on the perimeter of Patan are ascribed around, one at each corner of its cardinal points, which are popularly known as Asoka Stupas. Legend has it that Emperor Asoka (the legendary King of India) visited with his daughter Charumati to Kathmandu in 250 BC and erected five Asoka Stupas, four in the surrounding and one at the middle of the Patan. The size and shape of these stupas seem to breathe their antiquity in a real sense. There are more than 1,200 Buddhist monuments of various shapes and sizes scattered in and around the city.

text: The city was initially designed in the shape of the

entity_name: Buddhism

text: Buddhist

text: Dharma-Chakra (Wheel of Righteousness). The four thurs or mounds on the perimeter of Patan are ascribed around, one at each corner of its cardinal points, which are popularly known as Asoka Stupas. Legend has it that Emperor

entity_name: Ashoka

text: Asoka

text: (the legendary King of

entity_name: India

text: India

text: ) visited with his daughter Charumati to

entity_name: Kathmandu

text: Kathmandu

text: in 250 BC and erected five Asoka Stupas, four in the surrounding and one at the middle of the Patan. The size and shape of these stupas seem to breathe their antiquity in a real sense. There are more than 1,200

text: Buddhist

text: monuments of various shapes and sizes scattered in and around the city.

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answers: NDQ_002634

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answers: NDQ_002635

answers: 0

answers: NDQ_002636

answers: 0

answers: NDQ_002598

answers: various shapes and sizes

answers: NDQ_002599

answers: 1,200

answers: NDQ_002600

answers: stars

answers: NDQ_002601

answers: the shape of the Buddhist Dharma-Chakra

answers: NDQ_002602

answers: galaxies

answers: NDQ_002603

answers: elliptical galaxies

answers: NDQ_002604

answers: shape

answers: NDQ_002605

answers: stars

answers: NDQ_002606

answers: various shapes and sizes

answers: NDQ_002607

answers: are a type of star

answers: NDQ_002609

answers: 1,200

answers: NDQ_002610

answers: Wheel of Righteousness

answers: NDQ_002612

answers: Chakra

answers: NDQ_002615

answers: Chakra

answers: NDQ_002617

answers: Chakra

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: Chakra

answers: NDQ_002620

answers: Asoka Stupas

answers: NDQ_002621

answers: Chakra

answers: NDQ_002622

answers: Patan

answers: NDQ_002623

answers: Asoka Stupa

answers: NDQ_002624

answers: Chakra

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is rotating around our galaxy.

answers: NDQ_002627

answers: Asoka Stupas

answers: NDQ_002628

answers: Star clusters

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: various shapes

answers: NDQ_002631

answers: spiral galaxies

answers: NDQ_002632

answers: dwarf galaxies

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: The Dharma-Chakra

answers: NDQ_002635

answers: orbits the central disk of our galaxy

answers: NDQ_002636

answers: Wheel of Righteousness

text: IC 1526  is a spiral galaxy in Pisces

text: IC 1526  is a

entity_name: Spiral galaxy

text: spiral galaxy

text: in

entity_name: Pisces (constellation)

text: Pisces

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answers: 2: The answer has limited relevance and completeness, with noticeable gaps or inaccuracies.

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answers: star clusters

answers: NDQ_002599

answers: many stars

answers: NDQ_002600

answers: galaxies

answers: NDQ_002601

answers: spiral

answers: NDQ_002602

answers: spiral

answers: NDQ_002603

answers: elliptical galaxies are very thin.

answers: NDQ_002604

answers: spiral arms

answers: NDQ_002605

answers: galaxies

answers: NDQ_002606

answers: spiral

answers: NDQ_002607

answers: IC 1526 is a spiral galaxy

answers: NDQ_002609

answers: 4 billion stars

answers: NDQ_002610

answers: galaxy

answers: NDQ_002612

answers: spiral galaxy

answers: NDQ_002615

answers: spiral galaxy

answers: NDQ_002617

answers: spiral galaxy

answers: NDQ_002618

answers: The Milky Way is a spiral galaxy.

answers: NDQ_002619

answers: dwarf galaxy

answers: NDQ_002620

answers: spiral galaxies

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: spiral galaxy

answers: NDQ_002623

answers: Elliptical galaxies have older blue stars.

answers: NDQ_002624

answers: elliptical

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: IC 1526 is a spiral galaxy.

answers: NDQ_002627

answers: There are billions of galaxies in the universe

answers: NDQ_002628

answers: IC 1526 is a star cluster.

answers: NDQ_002629

answers: Open star clusters contain more stars.

answers: NDQ_002630

answers: spiral

answers: NDQ_002631

answers: elliptical galaxies

answers: NDQ_002632

answers: IC 1526 is a dwarf galaxy in Pisces.

answers: NDQ_002633

answers: IC 1526 is a spiral galaxy.

answers: NDQ_002634

answers: IC 1526 is a spiral galaxy.

answers: NDQ_002635

answers: Our solar system orbits the central disk of our galaxy.

answers: NDQ_002636

answers: IC 1526 is a spiral galaxy

text: The Milky Way runs through the constellation, featuring prominent objects such as the open cluster NGC 5823 and the planetary nebula NGC 5315. Circinus hosts a spiral galaxy, the Circinus Galaxy, which was discovered in 1977 and is the closest Seyfert galaxy to the Milky Way. The Alpha Circinids (ACI), a meteor shower also discovered in 1977, radiate from this constellation.

text: The

text: Milky Way

text: runs through the constellation, featuring prominent objects such as the

entity_name: Open cluster

text: open cluster

text: NGC 5823

text: and the

entity_name: Planetary nebula

text: planetary nebula

text: NGC 5315

text: . Circinus hosts a

text: spiral galaxy

text: , the

entity_name: Circinus Galaxy

text: Circinus Galaxy

text: , which was discovered in 1977 and is the closest

entity_name: Seyfert galaxy

text: Seyfert galaxy

text: to the Milky Way. The

text: Alpha Circinids

text: (ACI), a

entity_name: Meteor shower

text: meteor shower

text: also discovered in 1977, radiate from this constellation.

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answers: NDQ_002617

answers: Galaxy Note

answers: NDQ_002618

answers: The Galaxy Tab Pro series

answers: NDQ_002619

answers: galaxy

answers: NDQ_002620

answers: Galaxy Tab Pro

answers: NDQ_002621

answers: Galaxy

answers: NDQ_002622

answers: Galaxy Note

answers: NDQ_002623

answers: Galaxy Tab Pro

answers: NDQ_002624

answers: Galaxy

answers: NDQ_002625

answers: Galaxy Tab Pro

answers: NDQ_002626

answers: Galaxy

answers: NDQ_002627

answers: Galaxy Tab Pro

answers: NDQ_002628

answers: Galaxy Tab Pro

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: Galaxy Tab Pro

answers: NDQ_002631

answers: Galaxy Tab Pro

answers: NDQ_002632

answers: Galaxy Tab Pro

answers: NDQ_002633

answers: Galaxy Tab Pro

answers: NDQ_002634

answers: Galaxy

answers: NDQ_002635

answers: Our solar system orbits the central disk of our galaxy

answers: NDQ_002636

answers: Galaxy Tab Pro

text: To achieve the objectives set out above we have defined a representative sample of galaxies to study. The Herschel data alone does not provide us with a large completely sampled region of sky, but we can use the WISE data to define a near infrared selected sample. As many galaxy properties correlate first with stellar mass, the near infrared, where for most galaxies the bulk of the stellar radiation emerges, provides the best available choice for galaxy selection. There are 3045 galaxies with a WISE 3.4μm detection (SN > 3) within 3000 km s (≈40 Mpc) of the Sun and with a size of D>1 arc min (≈12 kpc at 40 Mpc) – the W sample. Currently within the Herschel archive there are 613 observations of galaxies from this W sample. The intersection of these two samples we will refer to as the WH sample. We will carry out a similar selection for galaxies detected by Planck once the final data becomes available in late 2013 and the intersection of this sample with the WH sample is the WHP sample. The WH sample consists of 80 early type galaxies (T< 0) and 533 late types, 70 of which may be described as star forming irregulars/dwarfs. Also, within the WH sample we have 94 galaxies that have D> 5 arc min and so are resolved in the Herschel bands and lend themselves to full radiative transfer and infrared/mm SED modelling.

text: To achieve the objectives set out above we have defined a representative sample of galaxies to study. The Herschel data alone does not provide us with a large completely sampled region of sky, but we can use the

entity_name: Wide-field Infrared Survey Explorer

text: WISE

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answers: NDQ_002598

answers: irregulars/dwarfs

answers: NDQ_002599

answers: 3045 galaxies

answers: NDQ_002600

answers: Stars

answers: NDQ_002601

answers: star forming

answers: NDQ_002602

answers: star forming irregulars/dwarfs

answers: NDQ_002603

answers: the bulk of the stellar radiation emerges

answers: NDQ_002604

answers: star forming irregulars/dwarfs

answers: NDQ_002605

answers: galaxies

answers: NDQ_002606

answers: irregulars/dwarfs

answers: NDQ_002607

answers: galaxies

answers: NDQ_002609

answers: 3045 galaxies

answers: NDQ_002610

answers: star

answers: NDQ_002612

answers: galaxies

answers: NDQ_002615

answers: galaxy

answers: NDQ_002617

answers: star forming irregulars

answers: NDQ_002618

answers: Herschel bands

answers: NDQ_002619

answers: dwarfs

answers: NDQ_002620

answers: Star forming irregulars/dwarfs

answers: NDQ_002621

answers: galaxies

answers: NDQ_002622

answers: galaxies

answers: NDQ_002623

answers: The WH sample consists of 80 early type galaxies

answers: NDQ_002624

answers: irregulars/dwarfs

answers: NDQ_002625

answers: 3045 galaxies with a WISE 3.4 m detection

answers: NDQ_002626

answers: The Sun is rotating around our galaxy.

answers: NDQ_002627

answers: There are 3045 galaxies with a WISE 3.4 m detection

answers: NDQ_002628

answers: galaxies

answers: NDQ_002629

answers: open star clusters

answers: NDQ_002630

answers: D>1 arc min

answers: NDQ_002631

answers: spiral galaxies

answers: NDQ_002632

answers: Dwarf galaxies are often found near larger galaxies.

answers: NDQ_002633

answers: The WISE data alone does not provide us with a large completely sampled region of sky

answers: NDQ_002634

answers: The Sun is within one of the spiral arms of our galaxy.

answers: NDQ_002635

answers: The Sun orbits the central disk of our galaxy.

answers: NDQ_002636

answers: galaxies

text: Since 2006, a series of massive clusters have been identified bear the base of the Crux-Scutum Arm of the galaxy, each containing multiple red supergiants.  RSGC1 contains at least 12 red supergiants, RSGC2 (also known as Stephenson 2) contains at least 26, RSGC3 contains at least 8, and RSGC4 (also known as Alicante 8) contains at least 8.  A total of 80 confirmed red supergiants have been identified within a small area of the sky in the direction of these clusters.  These four clusters appear to be part of a massive burst of star formation 10-20 million years ago at the near end of the bar at the centre of the galaxy.  Similar massive clusters have been found near the far end of the galactic bar, but not such large numbers of red supergiants.

text: Since 2006, a series of massive clusters have been identified bear the base of the

text: Crux-Scutum Arm

text: of the galaxy, each containing multiple red supergiants.

text: contains at least 12 red supergiants, RSGC2 (also known as

text: Stephenson 2

text: ) contains at least 26,

text: contains at least 8, and RSGC4 (also known as

text: Alicante 8

text: ) contains at least 8.  A total of 80 confirmed red supergiants have been identified within a small area of the sky in the direction of these clusters.  These four clusters appear to be part of a massive burst of star formation 10-20 million years ago at the near end of the bar at the centre of the galaxy.  Similar massive clusters have been found near the far end of the galactic bar, but not such large numbers of red supergiants.

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answers: NDQ_002626

answers: The Crux-Scutum Arm

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answers: Crux-Scutum

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text: The Local Group is the galaxy group that includes the Milky Way. The Local Group comprises more than 54 galaxies, most of them dwarf galaxies. Its gravitational center is located somewhere between the Milky Way and the Andromeda Galaxy. The Local Group covers a diameter of  (about 10 meters) and has a binary (dumbbell)distribution. The group itself is a part of the larger Virgo Supercluster, which in turn may be a part of the Laniakea Supercluster.

text: The Local Group is the

text: galaxy group

text: that includes the

text: Milky Way

text: . The Local Group comprises more than 54 galaxies, most of them

text: dwarf galaxies

text: . Its gravitational center is located somewhere between the Milky Way and the

text: Andromeda Galaxy

text: . The Local Group covers a diameter of  (about 10 meters) and has a binary (dumbbell)distribution. The group itself is a part of the larger

text: Virgo Supercluster

text: , which in turn may be a part of the

text: Laniakea Supercluster

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answers: Most of them dwarf galaxies

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text: NGC 4618 is a distorted barred dwarf galaxy in the constellation Canes Venatici.  The galaxy is formally classified as a Sm galaxy, which means that its structure vaguely resembles the structure of spiral galaxies.  The galaxy is sometimes referred to as a Magellanic spiral because of its resemblance to the Magellanic clouds.

text: NGC 4618 is a distorted barred

text: dwarf galaxy

text: in the

text: constellation

text: Canes Venatici

text: .  The galaxy is formally classified as a

text: Sm

text: galaxy, which means that its structure vaguely resembles the structure of

text: spiral galaxies

text: .  The galaxy is sometimes referred to as a

text: Magellanic spiral

text: because of its resemblance to the

text: Magellanic clouds

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answers: Milky Way Galaxy

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answers: galaxy is formally classified as a Sm galaxy

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answers: The galaxy is formally classified as a Sm galaxy

text: The Milky Way is the galaxy that contains our Solar System. Its name "milky" is derived from its appearance as a dim glowing band arching across the night sky whose individual stars cannot be distinguished by the naked eye. The term "Milky Way" is a translation of the Latin via lactea, from the Greek γαλαξίας κύκλος (, "milky circle"). From Earth, the Milky Way appears as a band because its disk-shaped structure is viewed from within. Galileo Galilei first resolved the band of light into individual stars with his telescope in 1610. Until the early 1920s, most astronomers thought that the Milky Way contained all the stars in the Universe. Following the 1920 Great Debate between the astronomers Harlow Shapley and Heber Curtis, observations by Edwin Hubble showed that the Milky Way is just one of many galaxies.  Subsequent sensitive observations such as the Hubble telescope's Ultra Deep Field revealed a myriad of faint galaxies, which led to an estimate that the observable universe contained about 200 billion galaxies.  A 2016 study estimated that the observable universe contained ten times that number or 2 trillion galaxies.

text: The Milky Way is the

text: galaxy

text: that contains our

text: Solar System

text: . Its name "milky" is derived from its appearance as a dim glowing band arching across the night sky whose individual stars cannot be distinguished by the naked eye. The term "Milky Way" is a translation of the

text: Latin

text: via lactea, from the

text: Greek

text: γαλαξίας κύκλος (, "milky circle"). From Earth, the Milky Way appears as a band because its disk-shaped structure is viewed from within.

text: Galileo Galilei

text: first resolved the band of light into individual stars with his telescope in 1610. Until the early 1920s, most astronomers thought that the Milky Way contained all the stars in the

text: Universe

text: . Following the 1920

text: Great Debate

text: between the astronomers

text: Harlow Shapley

text: and

text: Heber Curtis

text: , observations by

text: Edwin Hubble

text: showed that the Milky Way is just one of many galaxies.  Subsequent sensitive observations such as the Hubble telescope's

text: Ultra Deep Field

text: revealed a myriad of faint galaxies, which led to an estimate that the

text: observable universe

text: contained about 200 billion galaxies.  A 2016 study estimated that the observable universe contained ten times that number or 2 trillion galaxies.

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text: It is thought that Red Spirals are galaxies in the process of transition from young to old. They are more massive than blue spirals and are found on the outskirts of large clusters of galaxies. Chris Lintott stated: "We think what we’re seeing is galaxies that have been gently strangled, so to speak, where somehow the gas supply for star formation has been cut off, but that they’ve been strangled so gently that the arms are still there." The cause might be the Red Spiral's gentle interaction with a galaxy cluster. He further explained: "The kind of thing we’re imagining [is that] as the galaxy moves into a denser environment, there’s lot of gas in clusters as well as galaxies, and it’s possible the gas from the galaxy just gets stripped off by the denser medium it’s plowing into."

text: It is thought that Red Spirals are galaxies in the process of transition from young to old. They are more massive than blue spirals and are found on the outskirts of large

text: clusters

text: of galaxies. Chris Lintott stated: "We think what we’re seeing is galaxies that have been gently strangled, so to speak, where somehow the gas supply for star formation has been cut off, but that they’ve been strangled so gently that the arms are still there." The cause might be the Red Spiral's gentle interaction with a galaxy cluster. He further explained: "The kind of thing we’re imagining [is that] as the galaxy moves into a denser environment, there’s lot of gas in clusters as well as galaxies, and it’s possible the gas from the galaxy just gets stripped off by the denser medium it’s plowing into."

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answers: 4

answers: NDQ_002598

answers: large clusters

answers: NDQ_002599

answers: large clusters

answers: NDQ_002600

answers: gas

answers: NDQ_002601

answers: gently strangled

answers: NDQ_002602

answers: Red Spirals

answers: NDQ_002603

answers: star formation has been cut off

answers: NDQ_002604

answers: arms

answers: NDQ_002605

answers: gas

answers: NDQ_002606

answers: Spirals

answers: NDQ_002607

answers: large clusters of galaxies

answers: NDQ_002609

answers: galaxies

answers: NDQ_002610

answers: galaxy cluster

answers: NDQ_002612

answers: spiral

answers: NDQ_002615

answers: large clusters

answers: NDQ_002617

answers: blue spirals

answers: NDQ_002618

answers: galaxy cluster

answers: NDQ_002619

answers: cluster

answers: NDQ_002620

answers: large clusters of galaxies

answers: NDQ_002621

answers: clusters

answers: NDQ_002622

answers: large clusters

answers: NDQ_002623

answers: Blue Spirals

answers: NDQ_002624

answers: Spirals

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The cause might be the Red Spiral's gentle interaction with a galaxy cluster

answers: NDQ_002627

answers: It is thought that Red Spirals are galaxies

answers: NDQ_002628

answers: Galaxies

answers: NDQ_002629

answers: open star clusters

answers: NDQ_002630

answers: more massive than blue spirals

answers: NDQ_002631

answers: Red Spirals

answers: NDQ_002632

answers: on the outskirts of large clusters

answers: NDQ_002633

answers: large clusters of galaxies

answers: NDQ_002634

answers: Red Spirals

answers: NDQ_002635

answers: Our solar system orbits the central disk of our galaxy

answers: NDQ_002636

answers: blue spirals

text: In 2005, astronomers discovered a completely new type of star cluster in the Andromeda Galaxy, which is, in several ways, very similar to globular clusters. The new-found clusters contain hundreds of thousands of stars, a similar number to that found in globular clusters. The clusters share other characteristics with globular clusters such as stellar populations and metallicity. What distinguishes them from the globular clusters is that they are much larger – several hundred light-years across – and hundreds of times less dense. The distances between the stars are, therefore, much greater within the newly discovered extended clusters. Parametrically, these clusters lie somewhere between a globular cluster and a dwarf spheroidal galaxy.

text: dwarf spheroidal galaxy

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answers: globular clusters

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answers: hundreds of thousands

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answers: hundreds of thousands of stars

answers: NDQ_002601

answers: Parametrically

answers: NDQ_002602

answers: globular clusters

answers: NDQ_002603

answers: hundreds of times less dense

answers: NDQ_002604

answers: hundreds of times less dense

answers: NDQ_002605

answers: hundreds of times less dense

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answers: dwarf spheroidal

answers: NDQ_002607

answers: similar to globular clusters

answers: NDQ_002609

answers: hundreds of thousands of stars

answers: NDQ_002610

answers: globular cluster

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answers: spheroidal galaxy

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answers: globular clusters

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answers: spheroidal

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answers: The Milky Way

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answers: star cluster

answers: NDQ_002620

answers: globular cluster

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answers: star cluster

answers: NDQ_002622

answers: globular clusters

answers: NDQ_002623

answers: globular clusters

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answers: dwarf spheroidal

answers: NDQ_002625

answers: Milky Way Galaxy

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answers: Our solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: galaxy

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answers: galaxy

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answers: hundreds of thousands of stars

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answers: dwarf spheroidal galaxy

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answers: elliptical

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answers: dwarf spheroidal galaxy

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answers: hundreds of thousands of stars

answers: NDQ_002634

answers: Galaxy

answers: NDQ_002635

answers: Galaxy

answers: NDQ_002636

answers: dwarf spheroidal

text: Spiral galaxies have central bar-shaped structures composed of stars. These galaxies are called 'barred spirals' and have been investigated by Galaxy Zoo in several studies. It is unclear why some spiral galaxies have bars and some do not. Galaxy Zoo research has shown that red spirals are about twice as likely to host bars as blue spirals. These colours are significant. Blue galaxies get their hue from the hot young stars they contain, implying that they are forming stars in large numbers. In red galaxies, this star formation has stopped, leaving behind the cooler, long-lived stars that give them their red colour.

text: Spiral galaxies

text: have central bar-shaped structures composed of stars. These galaxies are called

text: 'barred spirals'

text: and have been investigated by Galaxy Zoo in several studies. It is unclear why some spiral galaxies have bars and some do not. Galaxy Zoo research has shown that red spirals are about twice as likely to host bars as blue spirals. These colours are significant. Blue galaxies get their hue from the hot young stars they contain, implying that they are forming stars in large numbers. In red galaxies, this star formation has stopped, leaving behind the cooler, long-lived stars that give them their red colour.

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text: The Whirlpool Galaxy, also known as Messier 51a, M51a, or NGC 5194, is an interacting grand-design spiral galaxy with a Seyfert 2 active galactic nucleus in the constellation Canes Venatici. It was the first galaxy to be classified as a spiral galaxy. Recently it was estimated to be 23 ± 4 million light-years from the Milky Way, but different methods yield distances between 15 and 35 million light-years. Messier 51 is one of the best known galaxies in the sky.The galaxy and its companion, NGC 5195, are easily observed by amateur astronomers, and the two galaxies may even be seen with binoculars. The Whirlpool Galaxy is also a popular target for professional astronomers, who study it to further understand galaxy structure (particularly structure associated with the spiral arms) and galaxy interactions.

text: The Whirlpool Galaxy, also known as

text: Messier

text: 51a, M51a, or NGC 5194, is an

text: interacting

text: grand-design

text: spiral galaxy

text: with a

text: Seyfert 2

text: active galactic nucleus

text: in the

text: constellation

text: Canes Venatici

text: . It was the first galaxy to be classified as a spiral galaxy. Recently it was estimated to be 23 ± 4 million

text: light-year

text: s from the

text: Milky Way

text: , but different methods yield distances between 15 and 35 million light-years. Messier 51 is one of the best known galaxies in the sky.The galaxy and its companion,

text: NGC 5195

text: , are easily observed by

text: amateur astronomers

text: , and the two galaxies may even be seen with

text: binoculars

text: . The Whirlpool Galaxy is also a popular target for professional astronomers, who study it to further understand galaxy structure (particularly structure associated with the

text: spiral arms

text: ) and galaxy interactions.

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text: A spiral galaxy is a type of galaxy characterized by a central bulge of old Population II stars surrounded by a rotating disc of younger Population I stars. A spiral galaxy maintains its spirals arms due to density wave theory.

text: A

text: spiral galaxy

text: is a type of

text: galaxy

text: characterized by a central

text: bulge

text: of old

text: Population II

text: star

text: s surrounded by a rotating disc of younger

text: Population I

text: stars. A spiral galaxy maintains its

text: spirals arms

text: due to

text: density wave theory

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text: Type Sm and Im galaxies have also been categorized as irregular galaxies with some structure (type Irr-1). Sm galaxies are typically disrupted and asymmetric. dSm galaxies are dwarf spiral galaxies or dwarf irregular galaxies, depending on categorization scheme.

text: Type Sm and Im galaxies have also been categorized as

text: irregular galaxies

text: with some structure (type Irr-1). Sm galaxies are typically disrupted and asymmetric. dSm galaxies are

text: dwarf spiral galaxies

text: or

text: dwarf irregular galaxies

text: , depending on categorization scheme.

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text: NGC 5247 is a face-on unbarred spiral galaxy located some 60 million light years away in the constellation Virgo. It most likely belongs to the Virgo Supercluster of galaxies; the same supercluster that hosts the Milky Way galaxy. This is a grand design spiral galaxy that displays no indications of distortion caused by interaction with other galaxies. It has two spiral arms that bifurcate after wrapping half way around the nucleus. The disk is estimated to be  in thickness and it is inclined by roughly 28° to the line of sight.

text: NGC 5247 is a face-on

text: unbarred spiral galaxy

text: located some 60 million

text: light year

text: s away in the

text: constellation

text: Virgo

text: . It most likely belongs to the

text: Virgo Supercluster

text: of galaxies; the same

text: supercluster

text: that hosts the

text: Milky Way

text: galaxy. This is a

text: grand design spiral galaxy

text: that displays no indications of distortion caused by

text: interaction

text: with other galaxies. It has two spiral arms that bifurcate after wrapping half way around the nucleus. The disk is estimated to be  in thickness and it is inclined by roughly 28° to the line of sight.

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answers: Supercluster

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answers: 60 million

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answers: Milky Way galaxy

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answers: interaction with other galaxies

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answers: spiral galaxy

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answers: interaction with other galaxies

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answers: two spiral arms

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answers: unbarred

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answers: unbarred

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answers: NGC 5247

answers: NDQ_002609

answers: 60 million light years

answers: NDQ_002610

answers: nucleus

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answers: spiral

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answers: NGC 5247

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answers: Milky Way galaxy

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answers: The Milky Way galaxy

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answers: Supercluster

answers: NDQ_002620

answers: Milky Way galaxy

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answers: Supercluster

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answers: Virgo Supercluster

answers: NDQ_002623

answers: Milky Way galaxy

answers: NDQ_002624

answers: Milky Way galaxy

answers: NDQ_002625

answers: Milky Way galaxy

answers: NDQ_002626

answers: The Milky Way galaxy

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answers: The Milky Way galaxy

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answers: Supercluster

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answers: Open star clusters

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answers: grand design

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answers: The Milky Way galaxy

answers: NDQ_002632

answers: Milky Way galaxy

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answers: The Milky Way galaxy

answers: NDQ_002634

answers: The Milky Way galaxy

answers: NDQ_002635

answers: Milky Way

answers: NDQ_002636

answers: Milky Way galaxy

text: Andromeda Galaxy was formed roughly 10 billion years ago from the collision and subsequent merger of smaller protogalaxies.This violent collision formed most of the galaxy's (metal-rich) galactic halo and extended disk. During this epoch, star formation would have been very high, to the point of becoming a luminous infrared galaxy for roughly 100 million years. Andromeda and the Triangulum Galaxy had a very close passage 2–4 billion years ago. This event produced high levels of star formation across the Andromeda Galaxy's disk – even some globular clusters – and disturbed M33's outer disk.

text: Andromeda Galaxy was formed roughly 10 billion years ago from the collision and subsequent merger of smaller

text: protogalaxies

text: .This violent collision formed most of the galaxy's (metal-rich)

text: galactic halo

text: and extended disk. During this epoch,

text: star formation

text: would have been

text: very high

text: , to the point of becoming a

text: luminous infrared galaxy

text: for roughly 100 million years. Andromeda and the

text: Triangulum Galaxy

text: had a very close passage 2–4 billion years ago. This event produced high levels of star formation across the Andromeda Galaxy's disk – even some globular clusters – and disturbed M33's outer disk.

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answers: globular clusters

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answers: globular clusters

answers: NDQ_002600

answers: metal-rich

answers: NDQ_002601

answers: violent collision

answers: NDQ_002602

answers: globular clusters

answers: NDQ_002603

answers: star formation would have been very high

answers: NDQ_002604

answers: halo

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answers: disk

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answers: globular clusters

answers: NDQ_002607

answers: Andromeda Galaxy's disk

answers: NDQ_002609

answers: 10 billion years

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answers: globular clusters

answers: NDQ_002612

answers: galaxy

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answers: globular clusters

answers: NDQ_002617

answers: globular

answers: NDQ_002618

answers: luminous infrared galaxy

answers: NDQ_002619

answers: protogalaxies

answers: NDQ_002620

answers: Andromeda Galaxy

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: globular clusters

answers: NDQ_002623

answers: Andromeda Galaxy

answers: NDQ_002624

answers: globular

answers: NDQ_002625

answers: Andromeda Galaxy

answers: NDQ_002626

answers: Our solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: The universe has billions of galaxies.

answers: NDQ_002628

answers: Galaxies

answers: NDQ_002629

answers: globular clusters

answers: NDQ_002630

answers: smaller protogalaxies

answers: NDQ_002631

answers: Andromeda Galaxy

answers: NDQ_002632

answers: Andromeda and the Triangulum Galaxy

answers: NDQ_002633

answers: Galaxy

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answers: Andromeda Galaxy

answers: NDQ_002635

answers: Andromeda Galaxy

answers: NDQ_002636

answers: Andromeda

text: of elliptical galaxies, first noted by the astronomers Sandra M. Faber and Robert Earl Jackson in 1976.    The original relation can be expressed mathematically as:

text: of

text: elliptical galaxies

text: , first noted by the astronomers

text: Sandra M. Faber

text: and

text: Robert Earl Jackson

text: in 1976.    The original relation can be expressed mathematically as:

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answers: 3: The answer has limited relevance and completeness, with noticeable gaps or inaccuracies.

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answers: 4 billion galaxies

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answers: The original relation can be expressed mathematically as:

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answers: Open star clusters contain more stars

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answers: dwarf galaxies are often found near larger galaxies

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answers: The solar system orbits the central disk

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text: Kapteyn's Star is distinctive in a number of other regards: it has a high radial velocity, orbits the Milky Way retrograde, and is the nearest known halo star to the Sun. It is a member of a moving group of stars that share a common trajectory through space, named the Kapteyn moving group. Based upon their element abundances, these stars may once have been members of Omega Centauri, a globular cluster that is thought to be the remnant of a dwarf galaxy that merged with the Milky Way. During this process, the stars in the group, including Kapteyn's Star, may have been stripped away as tidal debris.

text: Kapteyn's Star is distinctive in a number of other regards: it has a high radial velocity, orbits the

text: Milky Way

text: retrograde

text: , and is the nearest known

text: halo

text: star to the Sun. It is a member of a

text: moving group

text: of stars that share a common trajectory through space, named the Kapteyn moving group. Based upon their

text: element abundances

text: , these stars may once have been members of

text: Omega Centauri

text: , a

text: globular cluster

text: that is thought to be the remnant of a

text: dwarf galaxy

text: that merged with the Milky Way. During this process, the stars in the group, including Kapteyn's Star, may have been stripped away as tidal debris.

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answers: billions of stars

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text: Most elliptical galaxies are composed of older, low-mass stars, with a sparse interstellar medium and minimal star formation activity, and they tend to be surrounded by large numbers of globular clusters. Elliptical galaxies are believed to make up approximately 10–15% of galaxies in the Virgo Supercluster, and they are not the dominant type of galaxy in the universe overall. They are preferentially found close to the centers of galaxy clusters. Elliptical galaxies are (together with lenticular galaxies) also called "early-type" galaxies (ETG), due to their location in the Hubble sequence, and are found to be less common in the early Universe.

text: Most elliptical galaxies are composed of older,

text: low-mass stars

text: , with a sparse

text: interstellar medium

text: and minimal

text: star formation

text: activity, and they tend to be surrounded by large numbers of

text: globular cluster

text: s. Elliptical galaxies are believed to make up approximately 10–15% of galaxies in the

text: Virgo Supercluster

text: , and they are not the dominant type of galaxy in the universe overall. They are preferentially found close to the centers of

text: galaxy cluster

text: s. Elliptical galaxies are (together with

text: lenticular galaxies

text: ) also called "early-type" galaxies (ETG), due to their location in the

text: Hubble sequence

text: , and are found to be less common in the early

text: Universe

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answers: globular clusters

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answers: 10–15%

answers: NDQ_002600

answers: low-mass stars

answers: NDQ_002601

answers: their location in the Hubble sequence

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answers: elliptical

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answers: low-mass stars

answers: NDQ_002604

answers: low-mass stars

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answers: low-mass stars

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answers: lenticular

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answers: Large numbers of globular clusters

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answers: 10–15% of galaxies

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answers: globular cluster

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answers: lenticular

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answers: They are not the dominant type of galaxy

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answers: The Milky Way Galaxy

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answers: Our solar system is slowly spinning around our galaxy.

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answers: It is not the dominant type of galaxy in the universe overall

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answers: galaxy clusters

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text: Although the UKST was originally used to take photographs of the sky, traditional photographic glass (and film) became largely superseded by large electronic CCD detectors in the late 1990s, and after 2000 the UKST was used mostly for multi-object spectroscopy with the 6 degree Field (6dF) instrument. 6dF uses a robot to position up to 150 optical fibres on a metal plate mounted at the focal plane of the UKST, which then carry light from the targets to a spectrograph which sits on the floor of the dome. The 6dF Galaxy Survey (6dFGS), a redshift survey of 120,000 infrared-selected galaxies was completed in 2005, and from 2003-2013 the UKST then carried out the RAdial Velocity Experiment (RAVE) to measure the radial velocities and metallicities of around to 0.5 million stars in the Milky Way Galaxy.

text: Although the UKST was originally used to take

text: photographs

text: of the sky, traditional photographic glass (and film) became largely superseded by large electronic

text: CCD

text: detectors in the late 1990s, and after 2000 the UKST was used mostly for multi-object

text: spectroscopy

text: with the 6 degree Field (6dF) instrument. 6dF uses a robot to position up to 150

text: optical fibres

text: on a metal plate mounted at the

text: focal plane

text: of the UKST, which then carry light from the targets to a

text: spectrograph

text: which sits on the floor of the dome. The

text: 6dF Galaxy Survey

text: (6dFGS), a

text: redshift survey

text: of 120,000

text: infrared

text: -selected

text: galaxies

text: was completed in 2005, and from 2003-2013 the UKST then carried out the

text: RAdial Velocity Experiment

text: (RAVE) to measure the

text: radial velocities

text: and

text: metallicities

text: of around to 0.5 million stars in the

text: Milky Way Galaxy

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text: In SAIS the game players explore a "plausibly implausible" (fictional) region of the Milky Way galaxy called The Purple Void.

text: In SAIS the game players explore a "plausibly implausible" (fictional) region of the

text: Milky Way

text: galaxy

text: called The Purple Void.

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text: Because galaxy-size density fluctuations get washed out by free-streaming, "hot" dark matter implies that the first objects that can form are huge supercluster-size pancakes, which then fragment into galaxies. Deep-field observations show instead that galaxies formed first, followed by clusters and superclusters as galaxies clump together.

text: Because galaxy-size density fluctuations get washed out by free-streaming, "hot" dark matter implies that the first objects that can form are huge supercluster-size pancakes, which then fragment into galaxies.

text: Deep-field observations

text: show instead that galaxies formed first, followed by clusters and

text: superclusters

text: as galaxies clump together.

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text: The formation of globular clusters remains a poorly understood phenomenon and it remains uncertain whether the stars in a globular cluster form in a single generation or are spawned across multiple generations over a period of several hundred million years. In many globular clusters, most of the stars are at approximately the same stage in stellar evolution, suggesting that they formed at about the same time. However, the star formation history varies from cluster to cluster, with some clusters showing distinct populations of stars. An example of this is the globular clusters in the Large Magellanic Cloud (LMC) that exhibit a bimodal population. During their youth, these LMC clusters may have encountered giant molecular clouds that triggered a second round of star formation. This star-forming period is relatively brief, compared to the age of many globular clusters.It has also been proposed that the reason for this multiplicity in stellar populations could have a dynamical origin. In the Antennae galaxy, for example, the Hubble Space Telescope has observed clusters of clusters, regions in the galaxy that span hundreds of parsecs, where many of the clusters will eventually collide and merge. Many of them present a significant range in ages, hence possibly metallicities, and their merger could plausibly lead to clusters with a bimodal or even multiple distribution of populations.

text: The formation of globular clusters remains a poorly understood phenomenon and it remains uncertain whether the stars in a globular cluster form in a single generation or are spawned across multiple generations over a period of several hundred million years. In many globular clusters, most of the stars are at approximately the same stage in

text: stellar evolution

text: , suggesting that they formed at about the same time. However, the star formation history varies from cluster to cluster, with some clusters showing distinct populations of stars. An example of this is the globular clusters in the

text: Large Magellanic Cloud

text: (LMC) that exhibit a bimodal population. During their youth, these LMC clusters may have encountered

text: giant molecular cloud

text: s that triggered a second round of star formation. This star-forming period is relatively brief, compared to the age of many globular clusters.It has also been proposed that the reason for this multiplicity in stellar populations could have a dynamical origin. In the

text: Antennae galaxy

text: , for example, the Hubble Space Telescope has observed clusters of clusters, regions in the galaxy that span hundreds of parsecs, where many of the clusters will eventually collide and merge. Many of them present a significant range in ages, hence possibly

text: metallicities

text: , and their merger could plausibly lead to clusters with a bimodal or even multiple distribution of populations.

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answers: NDQ_002598

answers: globular clusters

answers: NDQ_002599

answers: several hundred million

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answers: galaxies

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answers: many of the clusters will eventually collide and merge

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answers: galaxies

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answers: globular clusters

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answers: clusters of clusters

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answers: at approximately the same stage in stellar evolution

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answers: Clouds

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answers: formation of globular clusters remains a poorly understood phenomenon

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answers: hundreds of parsecs

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answers: globular clusters

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answers: galaxy

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answers: globular clusters

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answers: Large Magellanic Cloud

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answers: galaxy

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answers: globular cluster

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answers: clusters

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answers: globular clusters

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answers: globular clusters

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answers: globular

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answers: Milky Way Galaxy

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answers: It has been proposed that the reason for this multiplicity in stellar populations could have a dynamical origin

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answers: The formation of globular clusters remains a poorly understood phenomenon

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answers: The formation of globular clusters

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answers: Antennae galaxy

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answers: Galaxy

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answers: galaxy

text: Spiral galaxies consist of five distinct components:

text: Spiral galaxies consist of five distinct components:

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answers: star clusters

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answers: Spiral

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answers: spiral

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answers: elliptical galaxies

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answers: Spiral

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answers: Spiral galaxies

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answers: Elliptical

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answers: Spiral galaxies consist of five distinct components

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answers: Open star clusters contain more stars.

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answers: Stars

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answers: The solar system orbits the central disk of our galaxy.

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answers: spiral galaxies

text: In 2012, she published her findings from a study into the evolution of stars within galaxies which themselves are members of galaxy clusters, using the Gemini North Observatory in Hawaii.  The research found that a galaxy's position within the galactic cluster affected stellar evolution within that galaxy: the closer a galaxy is to the center of a cluster, the sooner it stops forming new stars. The interpretation of this is that near the centre of the cluster, the large number of close galactic neighbours influence each other through gravitation to produce a sea of hot gas, and that hot gas seems to be the limiting factor that constrains new star formation. Mergers of galaxies also play a part: her forecasts of how our own Milky Way galaxy will merge with the Andromeda Galaxy and the two smaller Magellanic Cloud galaxies in several billion years have prompted further new studies into how that will affect the rates of star formation locally.

text: In 2012, she published her findings from a study into the evolution of stars within galaxies which themselves are members of galaxy clusters, using the

text: Gemini North

text: Observatory in

text: Hawaii

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answers: galaxy clusters

answers: NDQ_002599

answers: several billion years

answers: NDQ_002600

answers: hot gas

answers: NDQ_002601

answers: Mergers of galaxies

answers: NDQ_002602

answers: Milky Way galaxy

answers: NDQ_002603

answers: galaxy's position within the galactic cluster

answers: NDQ_002604

answers: galaxy clusters

answers: NDQ_002605

answers: galaxies

answers: NDQ_002606

answers: galaxy clusters

answers: NDQ_002607

answers: galaxy clusters

answers: NDQ_002609

answers: billion stars

answers: NDQ_002610

answers: sea of hot gas

answers: NDQ_002612

answers: Milky Way galaxy

answers: NDQ_002615

answers: galaxy clusters

answers: NDQ_002617

answers: Milky Way

answers: NDQ_002618

answers: Galaxy clusters

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answers: galaxy clusters

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answers: Milky Way galaxy

answers: NDQ_002621

answers: galaxy clusters

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answers: galaxy clusters

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answers: galaxy clusters

answers: NDQ_002624

answers: Magellanic Cloud

answers: NDQ_002625

answers: Milky Way galaxy

answers: NDQ_002626

answers: Milky Way galaxy

answers: NDQ_002627

answers: galaxy clusters

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answers: galaxy clusters

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answers: Galaxy clusters

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answers: Milky Way galaxy

answers: NDQ_002635

answers: Milky Way

answers: NDQ_002636

answers: Milky Way galaxy

text: Galaxies come in three main types: ellipticals, spirals, and irregulars. A slightly more extensive description of galaxy types based on their appearance is given by the Hubble sequence. Since the Hubble sequence is entirely based upon visual morphological type(shape), it may miss certain important characteristics of galaxies such as star formation rate in starburst galaxies and activity in the cores of active galaxies.

text: Galaxies come in three main types: ellipticals, spirals, and irregulars. A slightly more extensive description of galaxy types based on their appearance is given by the

text: Hubble sequence

text: . Since the Hubble sequence is entirely based upon visual morphological type(shape), it may miss certain important characteristics of galaxies such as

text: star formation

text: rate in

text: starburst galaxies

text: and activity in the cores of

text: active galaxies

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answers: NDQ_002598

answers: starburst

answers: NDQ_002599

answers: active galaxies

answers: NDQ_002600

answers: star

answers: NDQ_002601

answers: Hubble sequence

answers: NDQ_002602

answers: ellipticals

answers: NDQ_002603

answers: star formation

answers: NDQ_002604

answers: galaxy types

answers: NDQ_002605

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answers: NDQ_002606

answers: irregulars

answers: NDQ_002607

answers: galaxies

answers: NDQ_002609

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answers: NDQ_002610

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answers: NDQ_002612

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answers: NDQ_002615

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answers: NDQ_002617

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answers: NDQ_002619

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answers: NDQ_002620

answers: ellipticals

answers: NDQ_002621

answers: Galaxies

answers: NDQ_002622

answers: galaxy

answers: NDQ_002623

answers: The Hubble sequence

answers: NDQ_002624

answers: irregulars

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The solar system is rotating around our galaxy.

answers: NDQ_002627

answers: galaxy types based on their appearance

answers: NDQ_002628

answers: Star clusters

answers: NDQ_002629

answers: open star clusters

answers: NDQ_002630

answers: It may miss certain important characteristics of galaxies

answers: NDQ_002631

answers: The Hubble sequence

answers: NDQ_002632

answers: dwarf galaxies

answers: NDQ_002633

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answers: NDQ_002634

answers: Spirals

answers: NDQ_002635

answers: Galaxies

answers: NDQ_002636

answers: Spirals

text: A barred spiral galaxy is a spiral galaxy with a central bar-shaped structure composed of stars. Bars are found in approximately two-thirds of all spiral galaxies. Bars generally affect both the motions of stars and interstellar gas within spiral galaxies and can affect spiral arms as well. The Milky Way Galaxy, where our own Solar System is located, is classified as a barred spiral galaxy.

text: A barred spiral galaxy is a

text: spiral galaxy

text: with a central bar-shaped structure composed of

text: star

text: s. Bars are found in approximately two-thirds of all spiral galaxies. Bars generally affect both the motions of stars and

text: interstellar gas

text: within spiral galaxies and can affect

text: spiral arm

text: s as well. The

text: Milky Way Galaxy

text: , where our own

text: Solar System

text: is located, is classified as a barred spiral galaxy.

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answers: NDQ_002627

answers: 4

answers: NDQ_002628

answers: 0

answers: NDQ_002629

answers: 3

answers: NDQ_002630

answers: 0

answers: NDQ_002631

answers: 4

answers: NDQ_002632

answers: 2

answers: NDQ_002633

answers: 4

answers: NDQ_002634

answers: 4

answers: NDQ_002635

answers: 4

answers: NDQ_002636

answers: 4

answers: NDQ_002598

answers: stars

answers: NDQ_002599

answers: approximately two-thirds

answers: NDQ_002600

answers: stars

answers: NDQ_002601

answers: bar-shaped structure

answers: NDQ_002602

answers: A barred spiral galaxy

answers: NDQ_002603

answers: stars

answers: NDQ_002604

answers: Bars

answers: NDQ_002605

answers: stars

answers: NDQ_002606

answers: barred

answers: NDQ_002607

answers: can affect spiral arms as well

answers: NDQ_002609

answers: stars

answers: NDQ_002610

answers: Bars

answers: NDQ_002612

answers: spiral galaxy

answers: NDQ_002615

answers: galaxy

answers: NDQ_002617

answers: Milky Way Galaxy

answers: NDQ_002618

answers: Stars

answers: NDQ_002619

answers: Solar System

answers: NDQ_002620

answers: The Milky Way Galaxy

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxy

answers: NDQ_002623

answers: The Milky Way Galaxy

answers: NDQ_002624

answers: barred spiral galaxy

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: The Milky Way Galaxy

answers: NDQ_002627

answers: The Milky Way Galaxy

answers: NDQ_002628

answers: Stars

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: The Milky Way Galaxy

answers: NDQ_002631

answers: Spiral galaxies

answers: NDQ_002632

answers: The Milky Way Galaxy

answers: NDQ_002633

answers: The Milky Way Galaxy

answers: NDQ_002634

answers: Spiral arms

answers: NDQ_002635

answers: Milky Way Galaxy

answers: NDQ_002636

answers: Milky Way Galaxy

text: Our own Galaxy, the Milky Way, is contained in the Local Group of more than 40 galaxies.

text: Our own Galaxy, the

text: Milky Way

text: , is contained in the

text: Local Group

text: of more than 40 galaxies.

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answers: 0

answers: tqa2:L_0062/T_0630/8e316475fbd7ea853c7290bba40e5bcd

answers: 3: The answer has limited relevance and completeness, with noticeable gaps or inaccuracy.

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answers: 2

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answers: 0

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answers: 0

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answers: 0

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answers: 0

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answers: 0

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answers: 0

answers: tqa2:L_0062/T_0632/76a4d20633cfa7e3d87362f8d2ec771b

answers: 0

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answers: 0

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answers: 0

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answers: 0

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answers: 0

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answers: 0

answers: NDQ_002598

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answers: NDQ_002599

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answers: NDQ_002600

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answers: NDQ_002601

answers: 0

answers: NDQ_002602

answers: 4

answers: NDQ_002603

answers: 0

answers: NDQ_002604

answers: 0

answers: NDQ_002605

answers: 0

answers: NDQ_002606

answers: 0

answers: NDQ_002607

answers: 0

answers: NDQ_002609

answers: 4

answers: NDQ_002610

answers: 0

answers: NDQ_002612

answers: 0

answers: NDQ_002615

answers: 0

answers: NDQ_002617

answers: 0

answers: NDQ_002618

answers: 4

answers: NDQ_002619

answers: 0

answers: NDQ_002620

answers: 2

answers: NDQ_002621

answers: 0

answers: NDQ_002622

answers: 0

answers: NDQ_002623

answers: 2

answers: NDQ_002624

answers: 0

answers: NDQ_002625

answers: 0

answers: NDQ_002626

answers: 4

answers: NDQ_002627

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answers: NDQ_002628

answers: 4

answers: NDQ_002629

answers: 3

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answers: 2

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answers: 2

answers: NDQ_002633

answers: 4

answers: NDQ_002634

answers: 4

answers: NDQ_002635

answers: 4

answers: NDQ_002636

answers: 4

answers: NDQ_002598

answers: Galaxies

answers: NDQ_002599

answers: more than 40

answers: NDQ_002600

answers: Milky Way

answers: NDQ_002601

answers: Local Group

answers: NDQ_002602

answers: Milky Way

answers: NDQ_002603

answers: gas and dust

answers: NDQ_002604

answers: galaxy

answers: NDQ_002605

answers: Galaxies

answers: NDQ_002606

answers: Galaxies

answers: NDQ_002607

answers: galaxies

answers: NDQ_002609

answers: 40 galaxies

answers: NDQ_002610

answers: Milky Way

answers: NDQ_002612

answers: Milky Way

answers: NDQ_002615

answers: Galaxies

answers: NDQ_002617

answers: Milky Way

answers: NDQ_002618

answers: Milky Way

answers: NDQ_002619

answers: Local Group

answers: NDQ_002620

answers: Milky Way

answers: NDQ_002621

answers: galaxies

answers: NDQ_002622

answers: Local Group

answers: NDQ_002623

answers: Milky Way

answers: NDQ_002624

answers: Milky Way

answers: NDQ_002625

answers: Milky Way

answers: NDQ_002626

answers: The Milky Way

answers: NDQ_002627

answers: more than 40 galaxies

answers: NDQ_002628

answers: star cluster

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: Local Group

answers: NDQ_002631

answers: The Milky Way

answers: NDQ_002632

answers: Dwarf galaxies

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: The Milky Way

answers: NDQ_002635

answers: The Milky Way

answers: NDQ_002636

answers: Milky Way

text: As the name suggests, an elliptical galaxy has the cross-sectional shape of an ellipse. The stars move along random orbits with no preferred direction. These galaxies contain little or no interstellar dust, few star-forming regions, and generally older stars. Elliptical galaxies are more commonly found at the core of galactic clusters, and may have been formed through mergers of large galaxies.

text: As the name suggests, an elliptical galaxy has the cross-sectional shape of an

text: ellipse

text: . The stars move along

text: random

text: orbits with no preferred direction. These galaxies contain little or no interstellar dust, few star-forming regions, and generally older stars. Elliptical galaxies are more commonly found at the core of galactic clusters, and may have been formed through mergers of large galaxies.

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answers: 4

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answers: 4

answers: tqa2:L_0062/T_0632/76a4d20633cfa7e3d87362f8d2ec771b

answers: 0

answers: tqa2:L_0062/T_0632/312dd58a52ea7bdc18423e16b71e736d

answers: 0

answers: tqa2:L_0062/T_0632/07df44424134e44a91809881a664b81a

answers: 0

answers: tqa2:L_0062/T_0632/24cc00a29e23692d56b0664eeefac3e9

answers: 4

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answers: 0

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answers: 0

answers: NDQ_002598

answers: 0

answers: NDQ_002599

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answers: NDQ_002600

answers: 4

answers: NDQ_002601

answers: 0

answers: NDQ_002602

answers: 4

answers: NDQ_002603

answers: 4

answers: NDQ_002604

answers: 0

answers: NDQ_002605

answers: 4

answers: NDQ_002606

answers: 4

answers: NDQ_002607

answers: 0

answers: NDQ_002609

answers: 0

answers: NDQ_002610

answers: 4

answers: NDQ_002612

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answers: NDQ_002615

answers: 0

answers: NDQ_002617

answers: 5

answers: NDQ_002618

answers: 0

answers: NDQ_002619

answers: 0

answers: NDQ_002620

answers: 4

answers: NDQ_002621

answers: 4

answers: NDQ_002622

answers: 4

answers: NDQ_002623

answers: 0

answers: NDQ_002624

answers: 0

answers: NDQ_002625

answers: 0

answers: NDQ_002626

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answers: NDQ_002627

answers: 4

answers: NDQ_002628

answers: 4

answers: NDQ_002629

answers: 3

answers: NDQ_002630

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answers: NDQ_002631

answers: 2

answers: NDQ_002632

answers: 3

answers: NDQ_002633

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answers: NDQ_002634

answers: 0

answers: NDQ_002635

answers: 0

answers: NDQ_002636

answers: 4

answers: NDQ_002598

answers: galactic clusters

answers: NDQ_002599

answers: large galaxies

answers: NDQ_002600

answers: stars

answers: NDQ_002601

answers: formed through mergers of large galaxies

answers: NDQ_002602

answers: elliptical galaxy

answers: NDQ_002603

answers: stars move along random orbits

answers: NDQ_002604

answers: cross-sectional shape of an ellipse

answers: NDQ_002605

answers: older stars

answers: NDQ_002606

answers: Elliptical

answers: NDQ_002607

answers: galactic clusters

answers: NDQ_002609

answers: stars

answers: NDQ_002610

answers: elliptical galaxy

answers: NDQ_002612

answers: galaxy

answers: NDQ_002615

answers: galactic cluster

answers: NDQ_002617

answers: elliptical

answers: NDQ_002618

answers: galaxy

answers: NDQ_002619

answers: clusters

answers: NDQ_002620

answers: Elliptical galaxies

answers: NDQ_002621

answers: galactic clusters

answers: NDQ_002622

answers: galactic clusters

answers: NDQ_002623

answers: no star-forming regions

answers: NDQ_002624

answers: galactic clusters

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: stars move along random orbits with no preferred direction

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: galactic clusters

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: large

answers: NDQ_002631

answers: Spiral

answers: NDQ_002632

answers: at the core of galactic clusters

answers: NDQ_002633

answers: galaxy

answers: NDQ_002634

answers: galaxy

answers: NDQ_002635

answers: galaxy

answers: NDQ_002636

answers: an ellipse

text: Not only was BX442 revealed to be a genuine spiral galaxy, but part of a sub-class known as 'grand-design' spirals.  Most spiral galaxies have subtler features and the arms of the spiral are not necessarily well-defined. A grand design spiral galaxy has very clearly well-formed and distinct arms that significantly stretch out around the galaxy center. Of all spiral galaxies, only about 10% of them are classified as a grand design spiral galaxy.

text: Not only was BX442 revealed to be a genuine spiral galaxy, but part of a sub-class known as 'grand-design' spirals.  Most spiral galaxies have subtler features and the arms of the spiral are not necessarily well-defined. A grand design spiral galaxy has very clearly well-formed and distinct arms that significantly stretch out around the galaxy center. Of all spiral galaxies, only about 10% of them are classified as a grand design spiral galaxy.

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answers: grand design spiral galaxy

answers: NDQ_002599

answers: galaxy

answers: NDQ_002600

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answers: NDQ_002601

answers: arms of the spiral are not necessarily well-defined

answers: NDQ_002602

answers: grand design spiral galaxy

answers: NDQ_002603

answers: elliptical

answers: NDQ_002604

answers: very clearly well-formed and distinct arms

answers: NDQ_002605

answers: galaxy

answers: NDQ_002606

answers: subtler features

answers: NDQ_002607

answers: are not necessarily well-defined

answers: NDQ_002609

answers: 10 billion stars

answers: NDQ_002610

answers: grand design spiral galaxy

answers: NDQ_002612

answers: spiral galaxy

answers: NDQ_002615

answers: galaxy

answers: NDQ_002617

answers: grand design spiral galaxy

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: sub-class

answers: NDQ_002620

answers: grand design spiral galaxy

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxy

answers: NDQ_002623

answers: Elliptical galaxies

answers: NDQ_002624

answers: grand-design galaxy

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The solar system is rotating around our galaxy.

answers: NDQ_002627

answers: BX442

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: open star clusters

answers: NDQ_002630

answers: sub-class

answers: NDQ_002631

answers: It's impossible to say

answers: NDQ_002632

answers: BX442

answers: NDQ_002633

answers: BX442

answers: NDQ_002634

answers: galaxy center

answers: NDQ_002635

answers: BX442

answers: NDQ_002636

answers: BX442

text: In the French astronomer Gérard de Vaucouleurs' revised Hubble Sandage (VRHS) system of galaxy morphological classification, the Triangulum galaxy is classified as type SA(s)cd. The S prefix indicates that it is a disk-shaped galaxy with prominent arms of gas and dust that spiral out from the nucleus—what is commonly known as a spiral galaxy. The A is assigned when the galactic nucleus lacks a bar-shaped structure, in contrast to SB class barred spiral galaxies. American astronomer Allan Sandage's "(s)" notation is used when the spiral arms emerge directly from the nucleus or central bar, rather than from an inner ring as with an (r)-type galaxy. Finally, the cd suffix represents a stage along the spiral sequence that describes the openness of the arms. A rating of cd indicates relatively loosely wound arms.

text: In the French astronomer

text: Gérard de Vaucouleurs

text: ' revised Hubble Sandage (VRHS) system of

text: galaxy morphological classification

text: , the Triangulum galaxy is classified as type SA(s)cd. The S prefix indicates that it is a disk-shaped galaxy with prominent arms of gas and dust that spiral out from the nucleus—what is commonly known as a

text: spiral galaxy

text: . The A is assigned when the galactic nucleus lacks a bar-shaped structure, in contrast to SB class

text: barred spiral galaxies

text: . American astronomer

text: Allan Sandage

text: 's "(s)" notation is used when the spiral arms emerge directly from the nucleus or central bar, rather than from an inner ring as with an (r)-type galaxy. Finally, the cd suffix represents a stage along the spiral sequence that describes the openness of the arms. A rating of cd indicates relatively loosely wound arms.

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answers: elliptical

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answers: prominent arms

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answers: loosely wound arms

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answers: galaxy

answers: NDQ_002617

answers: Triangulum

answers: NDQ_002618

answers: What is commonly known as a spiral galaxy

answers: NDQ_002619

answers: disk

answers: NDQ_002620

answers: galaxy morphological classification

answers: NDQ_002621

answers: galaxy

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answers: elliptical galaxies

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answers: Triangulum galaxy

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answers: S prefix indicates that it is a disk-shaped galaxy

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answers: galaxy

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answers: open star clusters

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answers: disk-shaped

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answers: The S prefix indicates that it is a disk-shaped galaxy

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answers: The Triangulum galaxy

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answers: galaxy

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answers: galaxy

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answers: what is commonly known as a spiral galaxy

text: The strength of diffusion damping is calculated by a mathematical expression for the damping factor, which figures into the Boltzmann equation, an equation which describes the amplitude of perturbations in the CMB. The strength of the diffusion damping is chiefly governed by the distance photons travel before being scattered (diffusion length). What affect the diffusion length are primarily the properties of the plasma in question: different sorts of plasma may experience different sorts of diffusion damping. The evolution of a plasma may also affect the damping process. The scale on which diffusion damping works is called the Silk scale and its value corresponds to the size of galaxies of the present day. The mass contained within the Silk scale is called the Silk mass and it corresponds to the mass of the galaxies.

text: The strength of diffusion damping is calculated by a mathematical expression for the damping factor, which figures into the

text: Boltzmann equation

text: , an equation which describes the amplitude of perturbations in the CMB. The strength of the diffusion damping is chiefly governed by the distance photons travel before being scattered (diffusion length). What affect the diffusion length are primarily the properties of the plasma in question: different sorts of plasma may experience different sorts of diffusion damping. The evolution of a plasma may also affect the damping process. The scale on which diffusion damping works is called the Silk scale and its value corresponds to the size of galaxies of the present day. The mass contained within the Silk scale is called the Silk mass and it corresponds to the mass of the galaxies.

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answers: NDQ_002602

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answers: NDQ_002603

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answers: NDQ_002604

answers: Diffusion length

answers: NDQ_002605

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answers: NDQ_002617

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answers: The Silk scale

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answers: NDQ_002626

answers: The Boltzmann equation describes the amplitude of perturbations

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answers: It corresponds to the mass of the galaxies

answers: NDQ_002628

answers: Star clusters

answers: NDQ_002629

answers: globular star clusters

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answers: NDQ_002631

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answers: The Silk scale

answers: NDQ_002635

answers: The Silk scale

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answers: The Silk scale

text: The theory accounts for the rotation curves of spiral galaxies, correctly reproducing the Tully-Fisher law.

text: The theory accounts for the rotation curves of spiral galaxies, correctly reproducing the

text: Tully-Fisher law

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answers: The Milky Way

answers: NDQ_002619

answers: galaxy

answers: NDQ_002620

answers: spiral galaxies

answers: NDQ_002621

answers: galaxies

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answers: galaxies

answers: NDQ_002623

answers: Tully-Fisher law

answers: NDQ_002624

answers: elliptical

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answers: Milky Way Galaxy

answers: NDQ_002626

answers: Tully-Fisher law

answers: NDQ_002627

answers: It accounts for the rotation curves

answers: NDQ_002628

answers: Star clusters

answers: NDQ_002629

answers: globular star clusters

answers: NDQ_002630

answers: spiral

answers: NDQ_002631

answers: Tully-Fisher law

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answers: Tully-Fisher law

answers: NDQ_002633

answers: Tully-Fisher law

answers: NDQ_002634

answers: The Tully-Fisher law

answers: NDQ_002635

answers: Tully-Fisher law

answers: NDQ_002636

answers: Tully-Fisher law

text: The Sculptor Wall is a superstructure of galaxies ("wall of galaxies") relatively near to the Milky Way Galaxy (redshift of approximately z=0.03), also known as the Sculptor superclusters.

text: The Sculptor Wall is a superstructure of

text: galaxies

text: "wall of galaxies"

text: ) relatively near to the

text: Milky Way Galaxy

text: redshift

text: of approximately z=0.03), also known as the Sculptor superclusters.

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answers: superclusters

answers: NDQ_002599

answers: galaxy

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answers: NDQ_002601

answers: redshift

answers: NDQ_002602

answers: superstructure

answers: NDQ_002603

answers: gas and dust

answers: NDQ_002604

answers: redshift

answers: NDQ_002605

answers: galaxies

answers: NDQ_002606

answers: superstructure

answers: NDQ_002607

answers: superstructure of galaxies

answers: NDQ_002609

answers: z=0.03

answers: NDQ_002610

answers: superclusters

answers: NDQ_002612

answers: Milky Way

answers: NDQ_002615

answers: superclusters

answers: NDQ_002617

answers: Milky Way Galaxy

answers: NDQ_002618

answers: The Milky Way Galaxy

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answers: superclusters

answers: NDQ_002620

answers: Milky Way Galaxy

answers: NDQ_002621

answers: superstructure

answers: NDQ_002622

answers: superclusters

answers: NDQ_002623

answers: The Sculptor Wall

answers: NDQ_002624

answers: superclusters

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The Milky Way Galaxy

answers: NDQ_002627

answers: The Milky Way Galaxy

answers: NDQ_002628

answers: superclusters

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: superstructure

answers: NDQ_002631

answers: Spiral galaxies

answers: NDQ_002632

answers: The Sculptor Wall

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answers: galaxies

answers: NDQ_002634

answers: Milky Way Galaxy

answers: NDQ_002635

answers: The Milky Way Galaxy

answers: NDQ_002636

answers: Milky Way Galaxy

text: Hepzibah is a brilliant natural athlete and acrobat, and skilled hand-to-hand combatant, trained in various forms of armed and unarmed combat known in the Shi'ar galaxy. She is also an expert marksman, and is knowledgeable in the operation of a wide variety of ship-sized weaponry. She is often armed with Shi'ar energy guns.

text: Hepzibah is a brilliant natural athlete and acrobat, and skilled hand-to-hand combatant, trained in various forms of armed and unarmed combat known in the Shi'ar galaxy. She is also an expert marksman, and is knowledgeable in the operation of a wide variety of ship-sized weaponry. She is often armed with Shi'ar energy guns.

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answers: NDQ_002621

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answers: NDQ_002622

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answers: Shi'ar

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answers: Shi'ar

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is rotating around our galaxy.

answers: NDQ_002627

answers: galaxy

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answers: Open star cluster

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answers: galaxy

answers: NDQ_002631

answers: Shi'ar

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answers: Shi'ar galaxy

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text: The cluster is a fairly heterogeneous mixture of spirals and ellipticals. , it is believed that the spirals of the cluster are distributed in an oblong prolate filament, approximately four times as long as it is wide, stretching along the line of sight from the Milky Way. The elliptical galaxies are more centrally concentrated than the spiral galaxies.

text: The cluster is a fairly

text: heterogeneous

text: mixture of spirals and ellipticals. , it is believed that the spirals of the cluster are distributed in an oblong

text: prolate

text: filament, approximately four times as long as it is wide, stretching along the line of sight from the

text: Milky Way

text: . The elliptical galaxies are more centrally concentrated than the spiral galaxies.

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answers: galaxies

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answers: approximately four times as long as it is wide

answers: NDQ_002600

answers: spirals

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answers: prolate filament

answers: NDQ_002602

answers: elliptical

answers: NDQ_002603

answers: they are more centrally concentrated

answers: NDQ_002604

answers: ellipticals

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answers: spirals

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answers: heterogeneous

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answers: elliptical galaxies

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answers: four times as long as it is wide

answers: NDQ_002610

answers: cluster

answers: NDQ_002612

answers: spiral

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answers: The Milky Way

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answers: galaxy

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answers: galaxies

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answers: The ellipticals are more centrally concentrated than the spiral galaxies

answers: NDQ_002624

answers: Milky Way

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answers: Milky Way Galaxy

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answers: The Milky Way

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answers: It is believed

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answers: Galaxies

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answers: The Milky Way

text: The Sculptor Galaxy (NGC 253) and a few other galaxies form a gravitationally-bound core in the center of this group.  A few other galaxies at the periphery may be associated with the group but may not be gravitationally bound.  Because most of the galaxies in this group are actually weakly gravitationally bound, the group may also be described as a filament. It is considered to be at an early stage of evolution in which galaxies are still falling into the group along filamentary structures.

text: The

text: Sculptor Galaxy

text: (NGC 253) and a few other galaxies form a gravitationally-bound core in the center of this group.  A few other galaxies at the periphery may be associated with the group but may not be gravitationally bound.  Because most of the galaxies in this group are actually weakly gravitationally bound, the group may also be described as a

text: filament

text: . It is considered to be at an early stage of evolution in which galaxies are still falling into the group along filamentary structures.

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answers: filamentary structures

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answers: filamentary structures

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answers: filamentary structures

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answers: gravitationally bound

answers: NDQ_002604

answers: filamentary structures

answers: NDQ_002605

answers: galaxies

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answers: galaxies

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answers: filamentary structures

answers: NDQ_002609

answers: galaxies

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answers: core

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answers: filamentary

answers: NDQ_002615

answers: galaxies

answers: NDQ_002617

answers: Sculptor Galaxy

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: filament

answers: NDQ_002620

answers: galaxies

answers: NDQ_002621

answers: filament

answers: NDQ_002622

answers: Sculptor Galaxy

answers: NDQ_002623

answers: galaxies are still falling into the group

answers: NDQ_002624

answers: Sculptor Galaxy

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The Sculptor Galaxy (NGC 253)

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: A star cluster

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: filamentary structures

answers: NDQ_002631

answers: spiral galaxies

answers: NDQ_002632

answers: dwarf galaxies

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: The Sculptor Galaxy

answers: NDQ_002635

answers: The Sculptor Galaxy

answers: NDQ_002636

answers: filamentary structures

text: DDO 216 (also known as Pegasus Dwarf Irregular Galaxy, PGC 71538 or UGC 12613) is a dwarf irregular galaxy located in the constellation Pegasus.

text: DDO 216

text: (also known as

text: Pegasus

text: Dwarf Irregular

text: Galaxy

text: PGC

text: 71538 or

text: UGC

text: 12613) is a

text: dwarf irregular galaxy

text: located in the

text: constellation

text: Pegasus

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answers: billions of stars

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answers: dwarf irregular galaxy

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answers: dwarf irregular galaxy

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answers: dwarf irregular galaxy

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answers: NDQ_002624

answers: dwarf irregular galaxy

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: DDO 216 is a dwarf irregular galaxy

answers: NDQ_002627

answers: The universe has billions of galaxies

answers: NDQ_002628

answers: A star cluster

answers: NDQ_002629

answers: Open star clusters

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answers: NDQ_002631

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answers: Pegasus

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answers: DDO 216 is a dwarf irregular galaxy

answers: NDQ_002635

answers: DDO 216

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answers: Pegasus

text: Leo A (also known as Leo III) is an irregular  galaxy that is part of the Local Group. It lies 2.6 million light-years from Earth, and was discovered by Fritz Zwicky in 1942. The estimated mass of this galaxy is  solar masses, with at least 80% consisting of an unknown dark matter. It is one of the most isolated galaxies in the Local Group and shows no indications of an interaction or merger for several billion years. However, Leo A is nearly unique among irregular galaxies in that more than 90% of its stars formed more recently than 8 billion years ago, suggesting a rather unusual evolutionary history. The presence of RR Lyrae variables shows that the galaxy has an old stellar population that is up to 10 billion years in age.

text: Leo A (also known as Leo III) is an

text: irregular

text: galaxy

text: that is part of the

text: Local Group

text: . It lies

text: million

text: light-year

text: s from

text: Earth

text: , and was discovered by

text: Fritz Zwicky

text: in 1942. The estimated mass of this galaxy is

text: solar mass

text: es, with at least 80% consisting of an unknown

text: dark matter

text: . It is one of the most isolated galaxies in the Local Group and shows no indications of an interaction or merger for several billion years. However, Leo A is nearly unique among irregular galaxies in that more than 90% of its stars formed more recently than 8 billion years ago, suggesting a rather unusual evolutionary history. The presence of

text: RR Lyrae variable

text: s shows that the galaxy has an old stellar population that is up to 10 billion years in age.

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answers: RR Lyrae

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answers: 10 billion years

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answers: dark matter

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answers: RR Lyrae variables

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answers: irregular

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answers: dark matter

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answers: old

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answers: RR Lyrae

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answers: galaxy

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answers: irregular galaxy

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answers: The Milky Way

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answers: Local Group

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answers: irregular galaxy

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answers: Local Group

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answers: galaxy

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answers: irregular galaxies

answers: NDQ_002624

answers: irregular galaxy

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The estimated mass of this galaxy is solar masses

answers: NDQ_002627

answers: The estimated mass of this galaxy is solar masses

answers: NDQ_002628

answers: Local Group

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: irregular

answers: NDQ_002631

answers: Leo A

answers: NDQ_002632

answers: Local Group

answers: NDQ_002633

answers: It lies 2.6 million light-years from Earth

answers: NDQ_002634

answers: Leo A

answers: NDQ_002635

answers: Earth

answers: NDQ_002636

answers: It lies 2.6 million light-years

text: Noah Brosch was fascinated very early in his scientific career by the unique appearance of Hoag's Object, a very round ring galaxy and published a number of papers on this topic. Together with his student Ido Finkelman, and with colleagues from Russia and the Netherlands, they showed that the visible ring is part of an even larger ring of neutral hydrogen and proposed that the ring represents material accreted by the elliptical core at least one billion years ago. Hoag's Object would, therefore, represent a much undisturbed galaxy .

text: Noah Brosch was fascinated very early in his scientific career by the unique appearance of

text: Hoag's Object

text: , a very round ring galaxy and published a number of papers on this topic. Together with his student Ido Finkelman, and with colleagues from Russia and the Netherlands, they showed that the visible ring is part of an even larger ring of neutral hydrogen and proposed that the ring represents material accreted by the elliptical core at least one billion years ago.

text: Hoag's Object

text: would, therefore, represent a much undisturbed galaxy .

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text: BX442 (Q2343-BX442) is a grand design spiral galaxy of type Sc. It has a companion dwarf galaxy. It is the most distant known grand design spiral galaxy in the universe, with a redshift of z=2.1765 ± 0.0001.Although commonly referred to as the oldest known grand design spiral galaxy in the universe,it is more accurately the earliest such galaxy known to exist in the universe, with a lookback time (the difference between the age of the universe now and the age of the universe at the time light left the galaxy) of 10.7 billion years in the concordance cosmology.  This time estimate means that structure seen in BX442 developed roughly 3 billion years after the Big Bang, and is 10 kiloparsecs (30,000 ly) in diameter.

text: BX442 (Q2343-BX442) is a

text: grand design

text: spiral

text: galaxy

text: of type

text: Sc

text: . It has a companion

text: dwarf galaxy

text: . It is the most distant known

text: grand design spiral galaxy

text: in the universe, with a redshift of z=2.1765 ± 0.0001.Although commonly referred to as the oldest known

text: grand design spiral galaxy

text: in the universe,it is more accurately the earliest such galaxy known to exist in the universe, with a lookback time (the difference between the age of the universe now and the age of the universe at the time light left the galaxy) of 10.7 billion years in the

text: concordance cosmology

text: .  This time estimate means that structure seen in BX442 developed roughly 3 billion years after the Big Bang, and is 10 kiloparsecs (30,000 ly) in diameter.

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answers: NDQ_002632

answers: companion dwarf galaxy

answers: NDQ_002633

answers: 10.7 billion years in the concordance cosmology

answers: NDQ_002634

answers: BX442

answers: NDQ_002635

answers: Our solar system orbits the central disk of our galaxy

answers: NDQ_002636

answers: BX442

text: The Magellanic Cloud galaxies were once classified as irregular galaxies. The Large Magellanic Cloud has since been re-classified as type SBm  a type of barred spiral galaxy, the barred Magellanic spiral type. The Small Magellanic Cloud remains classified as an irregular galaxy of type Im under current Galaxy morphological classification, although it does contain a bar structure.

text: The

text: Magellanic Cloud galaxies

text: were once classified as irregular galaxies. The

text: Large Magellanic Cloud

text: has since been re-classified as type SBm  a type of

text: barred spiral galaxy

text: , the barred

text: Magellanic spiral

text: type. The

text: Small Magellanic Cloud

text: remains classified as an irregular galaxy of type Im under current

text: Galaxy morphological classification

text: , although it does contain a

text: bar structure

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answers: NDQ_002598

answers: barred spiral

answers: NDQ_002599

answers: galaxy

answers: NDQ_002600

answers: bar structure

answers: NDQ_002601

answers: bar structure

answers: NDQ_002602

answers: barred spiral

answers: NDQ_002603

answers: barred spiral

answers: NDQ_002604

answers: bar structure

answers: NDQ_002605

answers: galaxy

answers: NDQ_002606

answers: irregular

answers: NDQ_002607

answers: barred spiral galaxy

answers: NDQ_002609

answers: galaxies

answers: NDQ_002610

answers: galaxy

answers: NDQ_002612

answers: spiral

answers: NDQ_002615

answers: galaxy

answers: NDQ_002617

answers: Small Magellanic Cloud

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: Small Magellanic Cloud

answers: NDQ_002620

answers: Small Magellanic Cloud

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxy

answers: NDQ_002623

answers: The Small Magellanic Cloud

answers: NDQ_002624

answers: Im

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The Magellanic Cloud

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: galaxies

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: The Large Magellanic Cloud

answers: NDQ_002631

answers: Spiral galaxies

answers: NDQ_002632

answers: Small Magellanic Cloud

answers: NDQ_002633

answers: Galaxy morphological classification

answers: NDQ_002634

answers: galaxy

answers: NDQ_002635

answers: Galaxy

answers: NDQ_002636

answers: type SBm

text: How these clusters are formed is not yet known, but their formation might well be related to that of globular clusters. Why M31 has such clusters, while the Milky Way has not, is not yet known. It is also unknown if any other galaxy contains this kind of clusters, but it would be very unlikely that M31 is the sole galaxy with extended clusters.

text: How these clusters are formed is not yet known, but their formation might well be related to that of globular clusters. Why M31 has such clusters, while the Milky Way has not, is not yet known. It is also unknown if any other galaxy contains this kind of clusters, but it would be very unlikely that M31 is the sole galaxy with extended clusters.

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answers: NDQ_002598

answers: extended clusters

answers: NDQ_002599

answers: galaxy

answers: NDQ_002600

answers: extended clusters

answers: NDQ_002601

answers: galaxy with extended clusters

answers: NDQ_002602

answers: Milky Way

answers: NDQ_002603

answers: the Milky Way has not

answers: NDQ_002604

answers: extended clusters

answers: NDQ_002605

answers: globular

answers: NDQ_002606

answers: galaxy

answers: NDQ_002607

answers: How these clusters are formed

answers: NDQ_002609

answers: billions of stars

answers: NDQ_002610

answers: extended clusters

answers: NDQ_002612

answers: Milky Way

answers: NDQ_002615

answers: extended clusters

answers: NDQ_002617

answers: Milky Way

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: clusters

answers: NDQ_002620

answers: Milky Way

answers: NDQ_002621

answers: clusters

answers: NDQ_002622

answers: extended clusters

answers: NDQ_002623

answers: The Milky Way

answers: NDQ_002624

answers: globular

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The Milky Way

answers: NDQ_002627

answers: It would be very unlikely that M31 is the sole galaxy

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: extended clusters

answers: NDQ_002631

answers: It is also unknown if any other galaxy contains this kind of clusters

answers: NDQ_002632

answers: The Milky Way

answers: NDQ_002633

answers: globular clusters

answers: NDQ_002634

answers: The Milky Way

answers: NDQ_002635

answers: The Milky Way

answers: NDQ_002636

answers: Milky Way

text: The mall was developed by Jacobs, Visconsi, and Jacobs Company of Cleveland, Ohio. Construction began September 18, 1970. Originally, the mall contained eight water pools and sunken lounge areas. Artists Clarence Van Duzer and Joseph McDonnell were commissioned to create art work for the mall. McDonnell created four sculptures, including a 3,000 pound metal yellow rhinoceros with red polka dots made of half-inch steel plates. Another was a 35'x22' chandelier-like work suspended above one of the entryways. The chandelier was multi-colored and according to McDonnell, was inspired by a game of pick-up sticks and designed to resemble "a galaxy of light" from outside the center. Van Duzen was responsible for the large central area with its  ceiling and four contemporary pillars. In the center was a large three-level pool with waterfalls, a  fountain, and flashing lights, all synchronized to music. The main entrance was flanked by sculpted stone blocks in relief with irregular shapes and sizes. All the water sculptures and sunken lounge areas were removed in the late 1980s and the main entrance was redesigned, with the addition of a food court.

text: The mall was developed by

text: Jacobs, Visconsi, and Jacobs Company

text: of

text: Cleveland, Ohio

text: . Construction began September 18, 1970. Originally, the mall contained eight water pools and sunken lounge areas. Artists Clarence Van Duzer and Joseph McDonnell were commissioned to create art work for the mall. McDonnell created four sculptures, including a 3,000 pound metal yellow

text: rhinoceros

text: with red polka dots made of half-inch steel plates. Another was a 35'x22'

text: chandelier

text: -like work suspended above one of the entryways. The chandelier was multi-colored and according to McDonnell, was inspired by a game of

text: pick-up sticks

text: and designed to resemble "a

text: galaxy

text: of light" from outside the center. Van Duzen was responsible for the large central area with its  ceiling and four contemporary pillars. In the center was a large three-level pool with waterfalls, a  fountain, and flashing lights, all synchronized to music. The main entrance was flanked by sculpted stone blocks in relief with irregular shapes and sizes. All the water sculptures and sunken lounge areas were removed in the late 1980s and the main entrance was redesigned, with the addition of a

text: food court

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answers: Our solar system is slowly spinning around our galaxy.

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answers: galaxy

answers: NDQ_002636

answers: galaxy of light

text: John Drury Clark was the first to present a spiral with an oval outline. His design was used as a vividly coloured two-page illustration in Life magazine for 16 May 1949. In 1951, Edgar Longman, an artist, not a chemist, painted a large mural, adapting the Life image  by making the shape elliptical and tilting it to produce a dynamic effect. This inspired Stewart, then 12 years old, with a love of chemistry. Having just read Fred Hoyle's book The Nature of the Universe, he had the idea that Longman's design resembled a spiral galaxy. He returned to the idea many years later and published a first version of his "galaxy" in November 2004. His design seeks to express the link between the utterly minute world of atoms and the vastness of the stars, in the interior of which the elements were forged, as Hoyle was the first to demonstrate in detail.

text: John Drury Clark

text: was the first to present a spiral with an oval outline. His design was used as a vividly coloured two-page illustration in Life magazine for 16 May 1949. In 1951,

text: Edgar Longman

text: , an artist, not a chemist, painted a large mural, adapting the Life image  by making the shape

text: elliptical

text: and tilting it to produce a dynamic effect. This inspired Stewart, then 12 years old, with a love of chemistry. Having just read

text: Fred Hoyle

text: 's book The Nature of the Universe, he had the idea that Longman's design resembled a

text: spiral galaxy

text: . He returned to the idea many years later and published a first version of his "galaxy" in November 2004. His design seeks to express the link between the utterly minute world of atoms and the vastness of the stars, in the interior of which the elements were forged, as Hoyle was the first to demonstrate in detail.

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answers: NDQ_002612

answers: spiral

answers: NDQ_002615

answers: galaxy

answers: NDQ_002617

answers: spiral

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: galaxy

answers: NDQ_002620

answers: galaxies

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxy

answers: NDQ_002623

answers: elliptical

answers: NDQ_002624

answers: galaxies

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The elements were forged

answers: NDQ_002627

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answers: galaxy

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answers: Open star clusters

answers: NDQ_002630

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answers: Stars

answers: NDQ_002634

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answers: NDQ_002636

answers: Edgar Longman

text: The brightest elliptical galaxies often have low-density cores that are not well described by Sérsic's law.  The "core-Sérsic" family of models was introduced by A. Graham et al. and Trujillo et al.  and further developed by B. Terzić and A. Graham in 2005 to describe such galaxies.  Core-Sérsic models have an additional set of parameters that describe the core radius and core density.

text: The brightest elliptical galaxies often have low-density cores that are not well described by Sérsic's law.  The "core-Sérsic" family of models was introduced by A. Graham et al. and Trujillo et al.  and further developed by B. Terzić and A. Graham in 2005 to describe such galaxies.  Core-Sérsic models have an additional set of parameters that describe the core radius and core density.

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answers: NDQ_002602

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answers: NDQ_002604

answers: core radius and core density

answers: NDQ_002605

answers: low-density

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answers: brightest elliptical galaxies

answers: NDQ_002609

answers: billions of stars

answers: NDQ_002610

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answers: NDQ_002612

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answers: NDQ_002621

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answers: NDQ_002624

answers: core-Sérsic

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answers: NDQ_002634

answers: Sérsic's law

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answers: core

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answers: Sérsic's law

text: The Spiderweb Galaxy (PGC 2826829, MRC 1138-262) is an irregular galaxy with a redshift of 2.156, which is 10.6 billion light years away. It has been recently imaged by the Hubble Space Telescope. It is formed from dozens of smaller galaxies that were seen in the process of merging through mutual gravitational attraction.

text: The Spiderweb Galaxy (PGC 2826829, MRC 1138-262) is an

text: irregular galaxy

text: with a

text: redshift

text: of 2.156, which is 10.6 billion

text: light year

text: s away. It has been recently imaged by the

text: Hubble Space Telescope

text: . It is formed from dozens of smaller galaxies that were seen in the process of merging through mutual gravitational attraction.

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answers: dozens

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answers: mutual gravitational attraction

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answers: a redshift of 2.156

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answers: galaxy

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answers: dozens of smaller galaxies

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answers: 10.6 billion light years

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answers: The Spiderweb Galaxy

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answers: dozens

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answers: Hubble Space Telescope

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answers: galaxies

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answers: NDQ_002622

answers: The Spiderweb Galaxy

answers: NDQ_002623

answers: irregular

answers: NDQ_002624

answers: irregular galaxy

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: 10.6 billion light years away

answers: NDQ_002627

answers: 10.6 billion light years

answers: NDQ_002628

answers: dozens of smaller galaxies

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: irregular

answers: NDQ_002631

answers: The Spiderweb Galaxy

answers: NDQ_002632

answers: mutual gravitational attraction

answers: NDQ_002633

answers: 10.6 billion light years

answers: NDQ_002634

answers: The Spiderweb Galaxy

answers: NDQ_002635

answers: The Spiderweb Galaxy

answers: NDQ_002636

answers: redshift

text: Several bright galaxies are found in Ursa Major, including the pair Messier 81 (one of the brightest galaxies in the sky) and Messier 82 above the bear's head, and Pinwheel Galaxy (M101), a spiral northeast of η Ursae Majoris. The spiral galaxies Messier 108 and Messier 109 are also found in this constellation. The bright planetary nebula Owl Nebula (M97) can be found along the bottom of the bowl of the Big Dipper.

text: Several bright

text: galaxies

text: are found in Ursa Major, including the pair

text: Messier 81

text: (one of the brightest galaxies in the sky) and

text: Messier 82

text: above the bear's head, and

text: Pinwheel Galaxy

text: (M101), a spiral northeast of

text: η Ursae Majoris

text: . The

text: spiral galaxies

text: Messier 108

text: and

text: Messier 109

text: are also found in this constellation. The bright

text: planetary nebula

text: Owl Nebula

text: (M97) can be found along the bottom of the bowl of the Big Dipper.

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answers: 2: The answer has limited relevance and completeness, with significant gaps or inaccuracy.

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answers: NDQ_002598

answers: galaxies

answers: NDQ_002599

answers: galaxy

answers: NDQ_002600

answers: galaxy

answers: NDQ_002601

answers: spiral

answers: NDQ_002602

answers: spiral

answers: NDQ_002603

answers: elliptical

answers: NDQ_002604

answers: galaxy

answers: NDQ_002605

answers: galaxy

answers: NDQ_002606

answers: spiral

answers: NDQ_002607

answers: Ursae Majoris

answers: NDQ_002609

answers: 1 billion galaxies

answers: NDQ_002610

answers: Pinwheel Galaxy

answers: NDQ_002612

answers: spiral

answers: NDQ_002615

answers: Galaxy

answers: NDQ_002617

answers: Pinwheel Galaxy

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: nebula

answers: NDQ_002620

answers: spiral galaxies

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: Galaxy

answers: NDQ_002623

answers: Spiral

answers: NDQ_002624

answers: planetary

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: Star cluster

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: spiral galaxies

answers: NDQ_002631

answers: Spiral

answers: NDQ_002632

answers: Pinwheel Galaxy (M101)

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: Ursa Major

answers: NDQ_002635

answers: Galaxy

answers: NDQ_002636

answers: Pinwheel Galaxy

text: -- modelling of star clusters, galaxies, dark matter halos  and galaxy clusters;—constructing anisotropic galaxy models for studies of dynamical instabilities.

text: -- modelling of

text: star cluster

text: s,

text: galaxies

text: dark matter halo

text: s  and

text: galaxy cluster

text: s;—constructing anisotropic galaxy models for studies of dynamical

text: instabilities

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answers: NDQ_002598

answers: galaxies

answers: NDQ_002599

answers: galaxies

answers: NDQ_002600

answers: dark matter

answers: NDQ_002601

answers: anisotropic galaxy models

answers: NDQ_002602

answers: star clusters

answers: NDQ_002603

answers: anisotropic galaxy

answers: NDQ_002604

answers: anisotropic galaxy models

answers: NDQ_002605

answers: galaxies

answers: NDQ_002606

answers: anisotropic

answers: NDQ_002607

answers: star clusters

answers: NDQ_002609

answers: star clusters

answers: NDQ_002610

answers: dark matter halos

answers: NDQ_002612

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answers: NDQ_002615

answers: galaxy clusters

answers: NDQ_002617

answers: anisotropic galaxy

answers: NDQ_002618

answers: galaxy

answers: NDQ_002619

answers: star clusters

answers: NDQ_002620

answers: dwarf galaxies

answers: NDQ_002621

answers: galaxy clusters

answers: NDQ_002622

answers: galaxy clusters

answers: NDQ_002623

answers: galaxy clusters

answers: NDQ_002624

answers: anisotropic galaxy

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Anisotropic galaxy models

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: galaxy clusters

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: galaxies

answers: NDQ_002631

answers: galaxy clusters

answers: NDQ_002632

answers: dwarf galaxies

answers: NDQ_002633

answers: galaxy clusters

answers: NDQ_002634

answers: galaxy

answers: NDQ_002635

answers: Our solar system orbits the central disk of our galaxy

answers: NDQ_002636

answers: galaxy

text: DDO 70 (also known as Sextans B, PGC 28913 or UGC 5373) is an irregular galaxy which is in the constellation of Sextans. It is located 4.44 million light years away from Earth.

text: DDO 70

text: (also known as

text: Sextans

text: B,

text: PGC

text: 28913 or

text: UGC

text: 5373) is an

text: irregular galaxy

text: which is in the

text: constellation

text: of

text: Sextans

text: . It is located 4.44 million

text: light years

text: away from

text: Earth

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answers: 2: The answer has limited relevance and completeness, with noticeable gaps or inaccuracy.

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answers: irregular galaxy

answers: NDQ_002599

answers: galaxy

answers: NDQ_002600

answers: light years

answers: NDQ_002601

answers: irregular galaxy

answers: NDQ_002602

answers: irregular

answers: NDQ_002603

answers: irregular

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answers: irregular galaxy

answers: NDQ_002605

answers: galaxy

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answers: irregular

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answers: irregular galaxy

answers: NDQ_002609

answers: 4 billion stars

answers: NDQ_002610

answers: galaxy

answers: NDQ_002612

answers: irregular galaxy

answers: NDQ_002615

answers: galaxy

answers: NDQ_002617

answers: irregular

answers: NDQ_002618

answers: Sextans

answers: NDQ_002619

answers: constellation

answers: NDQ_002620

answers: irregular galaxy

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: irregular galaxy

answers: NDQ_002623

answers: irregular

answers: NDQ_002624

answers: irregular galaxy

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: 4.44 million light years away

answers: NDQ_002627

answers: The universe has billions of galaxies

answers: NDQ_002628

answers: star cluster

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: irregular

answers: NDQ_002631

answers: irregular

answers: NDQ_002632

answers: Sextans

answers: NDQ_002633

answers: 4.44 million light years away

answers: NDQ_002634

answers: Sextans

answers: NDQ_002635

answers: Earth orbits the central disk of our galaxy.

answers: NDQ_002636

answers: irregular galaxy

text: Most prior models of dark matter assumed it is composed of weakly interacting massive particles (also referred to as "WIMPs") that clump together through gravitational attraction only because the other forces between particles are too weak to affect their motion.  The SIDM picture proposes that the other forces are strong enough for the particles to scatter off one another in regions where they would otherwise pile up (forming what cosmologists call a "cusp") in the center of galaxies.  Also, the scattering would reduce the mass of dwarf galaxies in orbit around larger galaxies because the dark matter particles surrounding the larger galaxy would scatter and, thereby, strip off the dark matter surrounding the dwarf galaxy.  This idea is particularly interesting because there is astronomical evidence suggesting that galaxy cores are not cuspy, and the most massive galaxies predicted by simulations based on WIMPs are not observed.  If the SIDM picture is correct, searches for WIMP dark matter will find nothing, and different approaches will be needed to determine the identity of dark matter.

text: Most prior models of dark matter assumed it is composed of

text: weakly interacting massive particles

text: (also referred to as "WIMPs") that clump together through gravitational attraction only because the other forces between particles are too weak to affect their motion.  The

text: SIDM

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answers: NDQ_002598

answers: galaxies

answers: NDQ_002599

answers: most massive galaxies

answers: NDQ_002600

answers: dark matter

answers: NDQ_002601

answers: scattering would reduce the mass of dwarf galaxies in orbit around larger galaxies

answers: NDQ_002602

answers: dwarf galaxies

answers: NDQ_002603

answers: weakly interacting massive particles

answers: NDQ_002604

answers: dark matter

answers: NDQ_002605

answers: dark matter

answers: NDQ_002606

answers: dwarf

answers: NDQ_002607

answers: galaxies

answers: NDQ_002609

answers: dark matter

answers: NDQ_002610

answers: "cusp"

answers: NDQ_002612

answers: dwarf galaxy

answers: NDQ_002615

answers: dwarf galaxy

answers: NDQ_002617

answers: dwarf galaxy

answers: NDQ_002618

answers: dark matter

answers: NDQ_002619

answers: dwarf galaxy

answers: NDQ_002620

answers: weakly interacting massive particles

answers: NDQ_002621

answers: galaxies

answers: NDQ_002622

answers: dwarf galaxy

answers: NDQ_002623

answers: galaxies

answers: NDQ_002624

answers: dwarf

answers: NDQ_002625

answers: Dark matter

answers: NDQ_002626

answers: orbit around larger galaxies

answers: NDQ_002627

answers: galaxy cores are not cuspy

answers: NDQ_002628

answers: Star clusters

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: dwarf galaxies

answers: NDQ_002631

answers: galaxies

answers: NDQ_002632

answers: orbit around larger galaxies

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: galaxy

answers: NDQ_002635

answers: The SIDM picture

answers: NDQ_002636

answers: galaxies

text: The 1966 four-door sedan version of the Galaxie was also produced in Brazil under the names Galaxie, Galaxie 500, LTD and Landau from 1967 to 1983.

text: The 1966 four-door sedan version of the Galaxie was also produced in

text: Brazil

text: under the names Galaxie, Galaxie 500, LTD and

text: Landau

text: from 1967 to 1983.

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answers: galaxie

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answers: NDQ_002600

answers: galaxie

answers: NDQ_002601

answers: Galaxie 500

answers: NDQ_002602

answers: galaxie 500

answers: NDQ_002603

answers: elliptical

answers: NDQ_002604

answers: Galaxie

answers: NDQ_002605

answers: galaxie

answers: NDQ_002606

answers: Galaxie

answers: NDQ_002607

answers: Galaxie

answers: NDQ_002609

answers: billions of stars

answers: NDQ_002610

answers: galaxy

answers: NDQ_002612

answers: galaxie

answers: NDQ_002615

answers: Galaxie

answers: NDQ_002617

answers: Galaxie

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: galaxie

answers: NDQ_002620

answers: Galaxie

answers: NDQ_002621

answers: Galaxie

answers: NDQ_002622

answers: Galaxie

answers: NDQ_002623

answers: Galaxie

answers: NDQ_002624

answers: galaxie

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: Galaxie

answers: NDQ_002628

answers: Galaxie

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: sedan

answers: NDQ_002631

answers: Galaxie

answers: NDQ_002632

answers: Galaxie

answers: NDQ_002633

answers: Galaxie

answers: NDQ_002634

answers: Galaxie

answers: NDQ_002635

answers: Our solar system orbits the central disk

answers: NDQ_002636

answers: Galaxie

text: NGC 604 is an H II region inside the Triangulum Galaxy. It was discovered by William Herschel on September 11, 1784. It is one of the largest H II regions in the Local Group of galaxies; at the galaxy's estimated distance of 2.7 million light-years its longest diameter is roughly 1500 light years (460 parsecs), over 40 times the size of the visible portion of the Orion Nebula. It is over 6300 times more luminous than the Orion Nebula, and if it were at the same distance it would outshine Venus. Its gas is ionized by a cluster of massive stars at its center. with 200 stars of spectral type O and WR, a mass of 10 solar masses, and an age of 3.5 million years; however, unlike the Large Magellanic Cloud's Tarantula Nebula central cluster (R136), NGC 604's one is much less compact and more similar to a large stellar association, being considered the prototypical example of a Scaled OB Association (SOBA)

text: NGC 604 is an

text: H II region

text: inside the

text: Triangulum Galaxy

text: . It was discovered by

text: William Herschel

text: on September 11, 1784. It is one of the largest H II regions in the

text: Local Group

text: of galaxies; at the galaxy's estimated distance of 2.7 million

text: light-year

text: s its longest diameter is roughly 1500 light years (460

text: parsec

text: s), over 40 times the size of the visible portion of the

text: Orion Nebula

text: . It is over 6300 times more

text: luminous

text: than the Orion Nebula, and if it were at the same distance it would outshine

text: Venus

text: . Its gas is

text: ionized

text: by a cluster of massive

text: star

text: s at its center. with 200 stars of spectral type

text: O

text: and

text: WR

text: , a mass of 10

text: solar mass

text: es, and an age of 3.5 million years; however, unlike the

text: Large Magellanic Cloud

text: 's

text: Tarantula Nebula

text: central cluster (

text: ), NGC 604's one is much less compact and more similar to a large

text: stellar association

text: , being considered the prototypical example of a Scaled OB Association (SOBA)

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answers: 3: The answer has limited relevance and completeness, with noticeable gaps or inaccuracy.

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answers: 4

answers: NDQ_002598

answers: Scaled OB Association

answers: NDQ_002599

answers: 10 solar masses

answers: NDQ_002600

answers: stars

answers: NDQ_002601

answers: Scaled OB Association

answers: NDQ_002602

answers: the Local Group

answers: NDQ_002603

answers: stars at its center

answers: NDQ_002604

answers: galaxy

answers: NDQ_002605

answers: massive stars

answers: NDQ_002606

answers: galaxy

answers: NDQ_002607

answers: Scaled OB Association

answers: NDQ_002609

answers: 10 solar masses

answers: NDQ_002610

answers: Scaled OB Association

answers: NDQ_002612

answers: Local Group

answers: NDQ_002615

answers: Scaled OB Association

answers: NDQ_002617

answers: Triangulum Galaxy

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: Large Magellanic Cloud

answers: NDQ_002620

answers: Large Magellanic Cloud

answers: NDQ_002621

answers: cluster

answers: NDQ_002622

answers: a large stellar association

answers: NDQ_002623

answers: The Orion Nebula

answers: NDQ_002624

answers: Triangulum Galaxy

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: It is one of the largest H II regions in the Local Group

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: galaxies

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: H II regions

answers: NDQ_002631

answers: spiral galaxies

answers: NDQ_002632

answers: Smaller galaxies

answers: NDQ_002633

answers: It is one of the largest H II regions

answers: NDQ_002634

answers: Triangulum Galaxy

answers: NDQ_002635

answers: Our solar system orbits the central disk of our galaxy

answers: NDQ_002636

answers: Triangulum Galaxy

text: The Milky Way is the second-largest galaxy in the Local Group, with its stellar disk approximately  in diameter, and, on average, approximately  thick. As a guide to the relative physical scale of the Milky Way, if the Solar System out to Neptune were the size of a US quarter (), the Milky Way would be approximately the size of the continental United States. A ring-like filament of stars wrapping around the Milky Way may actually belong to the Milky Way itself, rippling above and below the relatively flat galactic plane. If so, that would mean a diameter of .

text: The Milky Way is the second-largest galaxy in the

text: Local Group

text: , with its stellar disk approximately  in diameter, and, on average, approximately  thick. As a guide to the relative physical scale of the Milky Way, if the Solar System out to

text: Neptune

text: were the size of a US quarter (), the Milky Way would be approximately the size of the continental United States. A ring-like filament of stars wrapping around the Milky Way may actually belong to the Milky Way itself, rippling above and below the relatively flat galactic plane. If so, that would mean a diameter of .

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answers: NDQ_002598

answers: ring-like filament

answers: NDQ_002599

answers: stars

answers: NDQ_002600

answers: stars

answers: NDQ_002601

answers: rippling above and below

answers: NDQ_002602

answers: The Milky Way

answers: NDQ_002603

answers: flat galactic plane

answers: NDQ_002604

answers: diameter

answers: NDQ_002605

answers: filament

answers: NDQ_002606

answers: flat

answers: NDQ_002607

answers: A ring-like filament of stars

answers: NDQ_002609

answers: stars

answers: NDQ_002610

answers: the Milky Way itself

answers: NDQ_002612

answers: galactic plane

answers: NDQ_002615

answers: filament of stars

answers: NDQ_002617

answers: The Milky Way

answers: NDQ_002618

answers: A ring-like filament of stars

answers: NDQ_002619

answers: Local Group

answers: NDQ_002620

answers: The Milky Way

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: A ring-like filament

answers: NDQ_002623

answers: The Milky Way

answers: NDQ_002624

answers: The Milky Way

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: The Solar System out to Neptune

answers: NDQ_002627

answers: The Milky Way is the second-largest galaxy

answers: NDQ_002628

answers: A ring-like filament

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: diameter

answers: NDQ_002631

answers: The Milky Way

answers: NDQ_002632

answers: The Milky Way

answers: NDQ_002633

answers: galaxy

answers: NDQ_002634

answers: The Milky Way

answers: NDQ_002635

answers: The Milky Way

answers: NDQ_002636

answers: ring-like filament of stars wrapping around the Milky Way

text: The thin disk is a structural component of certain galaxies. The Milky Way's thin disk is thought to extend up to  in the vertical axis and contributes about 85% of the stars in the Galactic plane. It can be set apart from the thick disc of a galaxy since the latter is composed of older population stars created at an earlier stage of the galaxy formation. Stars in the thin disk, on the other hand, are created as a result of gas accretion at the end stage of a galaxy formation.

text: The thin disk is a structural component of certain

text: galaxies

text: . The

text: Milky Way

text: 's thin disk is thought to extend up to  in the vertical axis and contributes about 85% of the stars in the Galactic plane. It can be set apart from the

text: thick disc

text: of a galaxy since the latter is composed of older population stars created at an earlier stage of the galaxy formation. Stars in the thin disk, on the other hand, are created as a result of gas accretion at the end stage of a galaxy formation.

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answers: galaxies

answers: NDQ_002599

answers: population stars

answers: NDQ_002600

answers: thin disk

answers: NDQ_002601

answers: gas accretion

answers: NDQ_002602

answers: The Milky Way

answers: NDQ_002603

answers: thin disk

answers: NDQ_002604

answers: thin disk

answers: NDQ_002605

answers: gas accretion

answers: NDQ_002606

answers: galaxy

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answers: Stars in the thin disk

answers: NDQ_002609

answers: stars

answers: NDQ_002610

answers: thick disc

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answers: Milky Way

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answers: The Milky Way

answers: NDQ_002618

answers: The Milky Way

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answers: thin disk

answers: NDQ_002620

answers: Milky Way

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxy

answers: NDQ_002623

answers: The thin disk

answers: NDQ_002624

answers: Milky Way

answers: NDQ_002625

answers: Milky Way

answers: NDQ_002626

answers: The Milky Way's thin disk

answers: NDQ_002627

answers: The Milky Way

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: Stars in the thin disk

answers: NDQ_002630

answers: thick disc

answers: NDQ_002631

answers: The Milky Way

answers: NDQ_002632

answers: The Milky Way

answers: NDQ_002633

answers: The Milky Way

answers: NDQ_002634

answers: Milky Way

answers: NDQ_002635

answers: The Milky Way

answers: NDQ_002636

answers: thick disc

text: This motion can cause confusion when looking at a solar or galactic spectrum, because the expected redshift based on the simple Hubble law will be obscured by the peculiar motion.  For example, the shape and size of the Virgo Cluster has been a matter of great scientific scrutiny due to the very large peculiar velocities of the galaxies in the cluster.

text: This motion can cause confusion when looking at a solar or galactic spectrum, because the expected redshift based on the simple Hubble law will be obscured by the peculiar motion.  For example, the shape and size of the

text: Virgo Cluster

text: has been a matter of great scientific scrutiny due to the very large peculiar velocities of the galaxies in the cluster.

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answers: galaxy

answers: NDQ_002599

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answers: NDQ_002600

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answers: NDQ_002601

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answers: NDQ_002602

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answers: NDQ_002603

answers: peculiar motion

answers: NDQ_002604

answers: peculiar motion

answers: NDQ_002605

answers: Galaxies

answers: NDQ_002606

answers: peculiar

answers: NDQ_002607

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answers: NDQ_002609

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answers: NDQ_002610

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answers: NDQ_002612

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answers: NDQ_002615

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answers: NDQ_002617

answers: Virgo Cluster

answers: NDQ_002618

answers: galactic spectrum

answers: NDQ_002619

answers: cluster

answers: NDQ_002620

answers: galactic

answers: NDQ_002621

answers: cluster

answers: NDQ_002622

answers: Virgo Cluster

answers: NDQ_002623

answers: galaxies in the cluster

answers: NDQ_002624

answers: Virgo

answers: NDQ_002625

answers: galactic

answers: NDQ_002626

answers: Our solar system is slowly spinning around our galaxy.

answers: NDQ_002627

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answers: NDQ_002628

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answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: Virgo Cluster

answers: NDQ_002631

answers: Spiral galaxies

answers: NDQ_002632

answers: galaxies in the cluster

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: Virgo

answers: NDQ_002635

answers: Our solar system orbits the central disk of our galaxy

answers: NDQ_002636

answers: The shape and size

text: Many characteristics of a galaxy are correlated. For example, as one would expect, a galaxy with a higher luminosity has a larger effective radius. The usefulness of these correlations is when a characteristic that can be determined without prior knowledge of the galaxy's distance (such as central velocity dispersion - the Doppler width of spectral lines in the central parts of the galaxy) can be correlated with a property, such as luminosity, that can be determined only for galaxies of a known distance. With this correlation, one can determine the distance to galaxies, a difficult task in astronomy.

text: Many characteristics of a galaxy are correlated. For example, as one would expect, a galaxy with a higher

text: luminosity

text: has a larger effective radius. The usefulness of these correlations is when a characteristic that can be determined without prior knowledge of the galaxy's distance (such as central velocity dispersion - the Doppler width of spectral lines in the central parts of the galaxy) can be correlated with a property, such as luminosity, that can be determined only for galaxies of a known distance. With this correlation, one can determine the distance to galaxies, a difficult task in astronomy.

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answers: NDQ_002602

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answers: NDQ_002603

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answers: NDQ_002604

answers: larger effective radius

answers: NDQ_002605

answers: luminosity

answers: NDQ_002606

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answers: NDQ_002607

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answers: NDQ_002612

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answers: larger effective radius

answers: NDQ_002618

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answers: effective radius

answers: NDQ_002620

answers: galaxy with a higher luminosity

answers: NDQ_002621

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answers: NDQ_002622

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answers: NDQ_002623

answers: galaxy

answers: NDQ_002624

answers: central velocity dispersion

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The solar system is rotating around our galaxy.

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: galaxies

answers: NDQ_002630

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answers: NDQ_002631

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answers: NDQ_002632

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answers: NDQ_002633

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answers: NDQ_002636

answers: galaxy

text: An ultra diffuse galaxy (UDG) is an extremely-low-density galaxy. Such a galaxy may have the same size as the Milky Way but a visible star count of only 1%. Their lack of luminosity is due to the lack of star-forming gas in the galaxy. This results in old stellar populations.

text: An ultra diffuse galaxy (UDG) is an extremely-low-density

text: galaxy

text: . Such a galaxy may have the same size as the

text: Milky Way

text: but a visible star count of only 1%. Their lack of luminosity is due to the lack of star-forming gas in the galaxy. This results in old stellar populations.

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answers: NDQ_002598

answers: old stellar populations

answers: NDQ_002599

answers: 1%

answers: NDQ_002600

answers: Milky Way

answers: NDQ_002601

answers: low-density

answers: NDQ_002602

answers: ultra diffuse galaxy (UDG)

answers: NDQ_002603

answers: old stellar populations

answers: NDQ_002604

answers: low-density

answers: NDQ_002605

answers: old

answers: NDQ_002606

answers: diffuse

answers: NDQ_002607

answers: are old stellar populations

answers: NDQ_002609

answers: 1%

answers: NDQ_002610

answers: Milky Way

answers: NDQ_002612

answers: Milky Way

answers: NDQ_002615

answers: stellar populations

answers: NDQ_002617

answers: Milky Way

answers: NDQ_002618

answers: visible star count

answers: NDQ_002619

answers: stellar populations

answers: NDQ_002620

answers: Milky Way

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: Milky Way

answers: NDQ_002623

answers: Milky Way

answers: NDQ_002624

answers: ultra diffuse galaxy

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The Milky Way

answers: NDQ_002627

answers: The Milky Way

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: UDG

answers: NDQ_002631

answers: spiral

answers: NDQ_002632

answers: Milky Way

answers: NDQ_002633

answers: The Milky Way

answers: NDQ_002634

answers: Milky Way

answers: NDQ_002635

answers: Milky Way

answers: NDQ_002636

answers: Milky Way

text: The NGC 4038 Group is a group of galaxies across Corvus and Crater. The group may contain between 13 and 27 galaxies. The best-known member is the Antennae peculiar galaxy, located 0.25 north of 31 Crateris.  It consists of two interacting galaxies—NGC 4038 and 4039—that appear to have a heart shape as seen from Earth. The name originates from the huge tidal tails that come off the ends of the two galaxies, formed because of the spiral galaxies' original rotation. Both original galaxies were spiral galaxies and are now experiencing extensive star formation due to the interaction of gas clouds. The galaxies are 45 million light-years from Earth and each has multiple ultraluminous X-ray sources, the source of which is unknown. Astronomers theorize that they may be a rare type of x-ray emitting binary stars or intermediate-mass black holes. The Antennae galaxies appear in a telescope at the 10th magnitude. SN 2004gt was a type Ic supernova that erupted on December 12, 2004. The progenitor was not identified from older images of the galaxy, and is either a type WC Wolf-Rayet star with a mass over 40 times that of the Sun, or a star 20 to 40 times as massive as the Sun in a binary star system. SN 2007sr was a Type Ia supernova event that peaked in brightness on  December 14, 2007. The galaxy has been identified as a good place to take detailed images in case of further supernovae.

text: The

text: NGC 4038 Group

text: is a

text: group of galaxies

text: across Corvus and Crater. The group may contain between 13 and 27 galaxies. The best-known member is the

text: Antennae

text: peculiar galaxy

text: , located 0.25 north of 31 Crateris.  It consists of two

text: interacting

text: galaxies—NGC 4038 and 4039—that appear to have a heart shape as seen from Earth. The name originates from the huge tidal tails that come off the ends of the two galaxies, formed because of the spiral galaxies' original rotation. Both original galaxies were

text: spiral galaxies

text: and are now experiencing extensive

text: star formation

text: due to the interaction of gas clouds. The galaxies are 45 million light-years from Earth and each has multiple

text: ultraluminous X-ray source

text: s, the source of which is unknown. Astronomers theorize that they may be a rare type of x-ray emitting

text: binary star

text: s or

text: intermediate-mass black hole

text: s. The Antennae galaxies appear in a telescope at the 10th magnitude.

text: SN 2004gt

text: was a

text: type Ic supernova

text: that erupted on December 12, 2004. The progenitor was not identified from older images of the galaxy, and is either a type WC

text: Wolf-Rayet star

text: with a mass over 40 times that of

text: the Sun

text: , or a star 20 to 40 times as massive as the Sun in a

text: binary star

text: system.

text: SN 2007sr

text: was a

text: Type Ia supernova

text: event that peaked in brightness on  December 14, 2007. The galaxy has been identified as a good place to take detailed images in case of further supernovae.

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answers: NDQ_002635

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answers: NDQ_002636

answers: 4

answers: NDQ_002598

answers: Antennae peculiar galaxy

answers: NDQ_002599

answers: 20 to 40 times as massive

answers: NDQ_002600

answers: gas clouds

answers: NDQ_002601

answers: tidal tails

answers: NDQ_002602

answers: spiral

answers: NDQ_002603

answers: star formation

answers: NDQ_002604

answers: huge tidal tails

answers: NDQ_002605

answers: gas clouds

answers: NDQ_002606

answers: peculiar

answers: NDQ_002607

answers: The group may contain between 13 and 27 galaxies

answers: NDQ_002609

answers: 27 galaxies

answers: NDQ_002610

answers: black holes

answers: NDQ_002612

answers: spiral

answers: NDQ_002615

answers: Antennae peculiar galaxy

answers: NDQ_002617

answers: heart shape

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: The NGC 4038 Group

answers: NDQ_002620

answers: spiral galaxies

answers: NDQ_002621

answers: The NGC 4038 Group

answers: NDQ_002622

answers: Antennae peculiar galaxy

answers: NDQ_002623

answers: Spiral galaxies

answers: NDQ_002624

answers: heart shape

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: It consists of two interacting galaxies

answers: NDQ_002627

answers: It consists of two interacting galaxies

answers: NDQ_002628

answers: The NGC 4038 Group

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: Type Ia

answers: NDQ_002631

answers: Spiral galaxies

answers: NDQ_002632

answers: Antennae peculiar galaxy

answers: NDQ_002633

answers: The group may contain between 13 and 27 galaxies

answers: NDQ_002634

answers: Corvus

answers: NDQ_002635

answers: Earth orbits the central disk of our galaxy

answers: NDQ_002636

answers: Both original galaxies were spiral galaxies

text: The 1960 Ford looked all-new with twin headlights riding in a scalloped-square front clip.  The Fairlane was now the base model in the full-sized lineup, along with the Fairlane 500, Galaxie and range-topping Starliner. The Station Wagon Series continued with Ranch Wagon, Country Sedan and Country Squire models. The elegant Starliner 2-door hardtop was Ford's choice for NASCAR racing.  The 1960 fullsize Fords abandoned the ostentatious ornamentation of the 1950s for a futuristic, sleek look.  Round taillights were replaced by half-moon shaped taillights for 1960 only.  There were tailfins still, but smaller ones – the focus of Ford's stylists abandoning, as did the rest of the industry, the aviation influences of the previous decade and instead capturing the new obsession – the Space Race.  The Galaxie name was particularly appealing to this trend, it seems. Windshield wipers were extended to cover more of the windshield. Ford also introduced the center rear fuel door lid.

text: The 1960 Ford looked all-new with twin headlights riding in a scalloped-square front clip.  The Fairlane was now the base model in the full-sized lineup, along with the Fairlane 500, Galaxie and range-topping Starliner. The Station Wagon Series continued with Ranch Wagon, Country Sedan and Country Squire models. The elegant Starliner 2-door

text: hardtop

text: was Ford's choice for

text: NASCAR

text: racing.  The 1960 fullsize Fords abandoned the ostentatious ornamentation of the 1950s for a futuristic, sleek look.  Round taillights were replaced by half-moon shaped taillights for 1960 only.  There were tailfins still, but smaller ones – the focus of Ford's stylists abandoning, as did the rest of the industry, the aviation influences of the previous decade and instead capturing the new obsession – the

text: Space Race

text: .  The Galaxie name was particularly appealing to this trend, it seems. Windshield wipers were extended to cover more of the windshield. Ford also introduced the center rear fuel door lid.

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answers: NDQ_002634

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answers: NDQ_002635

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answers: NDQ_002636

answers: 0

answers: NDQ_002598

answers: Galaxie

answers: NDQ_002599

answers: billions

answers: NDQ_002600

answers: Galaxie

answers: NDQ_002601

answers: scalloped-square front clip

answers: NDQ_002602

answers: Galaxie

answers: NDQ_002603

answers: elliptical

answers: NDQ_002604

answers: tailfins

answers: NDQ_002605

answers: stars

answers: NDQ_002606

answers: Galaxie

answers: NDQ_002607

answers: Space Race

answers: NDQ_002609

answers: 4 billion stars

answers: NDQ_002610

answers: Galaxie

answers: NDQ_002612

answers: Galaxie

answers: NDQ_002615

answers: Galaxie

answers: NDQ_002617

answers: Galaxie

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: Galaxie

answers: NDQ_002620

answers: Galaxie

answers: NDQ_002621

answers: Galaxie

answers: NDQ_002622

answers: Galaxie

answers: NDQ_002623

answers: Galaxie

answers: NDQ_002624

answers: Galaxie

answers: NDQ_002625

answers: The 1960 Ford

answers: NDQ_002626

answers: The 1960 Ford

answers: NDQ_002627

answers: Galaxie

answers: NDQ_002628

answers: Starliner

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: Galaxie

answers: NDQ_002631

answers: Galaxie

answers: NDQ_002632

answers: Galaxie

answers: NDQ_002633

answers: Galaxie

answers: NDQ_002634

answers: Galaxie

answers: NDQ_002635

answers: The 1960 Ford

answers: NDQ_002636

answers: Galaxie

text: A lenticular galaxy is a type of galaxy intermediate between an elliptical and a spiral galaxy in galaxy morphological classification schemes. Lenticular galaxies are disc galaxies (like spiral galaxies) that have used up or lost most of their interstellar matter and therefore have very little ongoing star formation. They may, however, retain significant dust in their disks. As a result, they consist mainly of aging stars (like elliptical galaxies). Because of their ill-defined spiral arms, if they are inclined face-on it is often difficult to distinguish between them and elliptical galaxies. Despite the morphological differences, lenticular and elliptical galaxies share common properties like spectral features and scaling relations. Both can be considered early-type galaxies that are passively evolving, at least in the local part of the Universe.

text: A lenticular galaxy is a type of

text: galaxy

text: intermediate between an

text: elliptical

text: and a

text: spiral galaxy

text: in

text: galaxy morphological classification

text: schemes. Lenticular galaxies are

text: disc galaxies

text: (like spiral galaxies) that have used up or lost most of their

text: interstellar matter

text: and therefore have very little ongoing

text: star formation

text: . They may, however, retain significant dust in their disks. As a result, they consist mainly of aging stars (like elliptical galaxies). Because of their ill-defined

text: spiral arm

text: s, if they are inclined face-on it is often difficult to distinguish between them and elliptical galaxies. Despite the morphological differences, lenticular and elliptical galaxies share common properties like spectral features and scaling relations. Both can be considered early-type galaxies that are passively evolving, at least in the local part of the Universe.

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answers: very little ongoing star formation

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answers: NDQ_002598

answers: aging stars

answers: NDQ_002599

answers: aging stars

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answers: stars

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answers: ill-defined spiral arms

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answers: elliptical

answers: NDQ_002603

answers: aging stars

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answers: aging stars

answers: NDQ_002606

answers: lenticular

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answers: are disc galaxies

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answers: the Universe

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answers: spiral galaxies

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answers: significant dust

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answers: NDQ_002618

answers: The Milky Way

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answers: disc galaxies

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answers: significant dust

answers: NDQ_002623

answers: aging stars

answers: NDQ_002624

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answers: NDQ_002625

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answers: NDQ_002626

answers: Both can be considered early-type galaxies

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answers: galaxy morphological classification schemes

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answers: open star clusters

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answers: Lenticular galaxies

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answers: Because of their ill-defined spiral arms

answers: NDQ_002633

answers: galaxy morphological classification schemes

answers: NDQ_002634

answers: disk galaxies

answers: NDQ_002635

answers: disk galaxies

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text: Size: For a body of fissile material in any given shape, increasing the size of the body increases the average distance that neutrons must travel before they can reach the surface and escape. Hence, increasing the size of the body increases the likelihood of fission and decreases the likelihood of leakage. Hence, for any given shape (and reflection conditions - see below) there will be a size that gives an exact balance between the rate of neutron production and the combined rate of absorption and leakage. This is the critical size.

text: Size: For a body of fissile material in any given shape, increasing the size of the body increases the average distance that neutrons must travel before they can reach the surface and escape. Hence, increasing the size of the body increases the likelihood of fission and decreases the likelihood of leakage. Hence, for any given shape (and reflection conditions - see below) there will be a size that gives an exact balance between the rate of neutron production and the combined rate of absorption and leakage. This is the critical size.

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answers: neutrons must travel

answers: NDQ_002604

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answers: neutrons

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answers: NDQ_002607

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answers: NDQ_002609

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answers: NDQ_002612

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answers: Our solar system is within one of the spiral arms of our galaxy.

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answers: orbits the central disk of our galaxy

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text: Zwicky also notes, in the same paper, that according to a tired light model a distance-redshift relationship would necessarily be present in the light from sources within our own galaxy (even if the redshift would be so small that it would be hard to measure), that do not appear under a recessional-velocity based theory. He writes, referring to sources of light within our galaxy: "It is especially desirable to determine the redshift independent of the proper velocities of the objects observed". Subsequent to this, astronomers have patiently mapped out the three-dimensional velocity-position phase space for the galaxy and found the redshifts and blueshifts of galactic objects to accord well with the statistical distribution of a spiral galaxy, eliminating the intrinsic redshift component as an effect.

text: Zwicky also notes, in the same paper, that according to a tired light model a distance-redshift relationship would necessarily be present in the light from sources within our own galaxy (even if the redshift would be so small that it would be hard to measure), that do not appear under a recessional-velocity based theory. He writes, referring to sources of light within our galaxy: "It is especially desirable to determine the redshift independent of the proper velocities of the objects observed". Subsequent to this, astronomers have patiently mapped out the three-dimensional velocity-position

text: phase space

text: for the galaxy and found the redshifts and blueshifts of galactic objects to accord well with the statistical distribution of a spiral galaxy, eliminating the

entity_section: Redshift periodicity and intrinsic redshifts

text: intrinsic redshift

text: component as an effect.

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answers: NDQ_002598

answers: spiral galaxy

answers: NDQ_002599

answers: galaxy

answers: NDQ_002600

answers: redshift

answers: NDQ_002601

answers: recessional-velocity

answers: NDQ_002602

answers: spiral galaxy

answers: NDQ_002603

answers: recessional-velocity

answers: NDQ_002604

answers: redshift

answers: NDQ_002605

answers: galaxy

answers: NDQ_002606

answers: galaxy

answers: NDQ_002607

answers: galaxy

answers: NDQ_002609

answers: billions of stars

answers: NDQ_002610

answers: recessional

answers: NDQ_002612

answers: spiral galaxy

answers: NDQ_002615

answers: galaxy

answers: NDQ_002617

answers: recessional-velocity

answers: NDQ_002618

answers: galaxy

answers: NDQ_002619

answers: galactic objects

answers: NDQ_002620

answers: spiral galaxy

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxy

answers: NDQ_002623

answers: The statistical distribution of a spiral galaxy

answers: NDQ_002624

answers: recessional-velocity

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: The statistical distribution of a spiral galaxy

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: globular star clusters

answers: NDQ_002630

answers: spiral

answers: NDQ_002631

answers: The statistical distribution of a spiral galaxy

answers: NDQ_002632

answers: dwarf galaxies

answers: NDQ_002633

answers: galaxy

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answers: galaxy

answers: NDQ_002635

answers: galaxy

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answers: galaxy

text: Dwarf elliptical galaxies, or dEs, are elliptical galaxies that are much smaller than others. They are classified as dE, and are quite common in galaxy groups and clusters, and are usually companions to other galaxies.

text: Dwarf elliptical galaxies, or dEs, are

text: elliptical galaxies

text: that are much smaller than others. They are classified as dE, and are quite common in galaxy groups and clusters, and are usually companions to other galaxies.

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answers: galaxy groups

answers: NDQ_002599

answers: Galaxies

answers: NDQ_002600

answers: galaxies

answers: NDQ_002601

answers: elliptical

answers: NDQ_002602

answers: elliptical

answers: NDQ_002603

answers: they are much smaller than others

answers: NDQ_002604

answers: spiral arms

answers: NDQ_002605

answers: galaxies

answers: NDQ_002606

answers: Dwarf

answers: NDQ_002607

answers: Galaxies

answers: NDQ_002609

answers: 1 billion galaxies

answers: NDQ_002610

answers: galaxy groups and clusters

answers: NDQ_002612

answers: elliptical

answers: NDQ_002615

answers: clusters

answers: NDQ_002617

answers: elliptical

answers: NDQ_002618

answers: galaxy groups and clusters

answers: NDQ_002619

answers: cluster

answers: NDQ_002620

answers: dwarf elliptical galaxies

answers: NDQ_002621

answers: clusters

answers: NDQ_002622

answers: clusters

answers: NDQ_002623

answers: It's impossible to say

answers: NDQ_002624

answers: dwarf

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: galaxy groups and clusters

answers: NDQ_002628

answers: clusters

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: elliptical

answers: NDQ_002631

answers: spiral galaxies

answers: NDQ_002632

answers: companions to other galaxies

answers: NDQ_002633

answers: galaxy groups and clusters

answers: NDQ_002634

answers: galaxy groups

answers: NDQ_002635

answers: galaxy

answers: NDQ_002636

answers: galaxy groups and clusters

text: The Sombrero Galaxy is an unbarred spiral galaxy.

text: The

text: Sombrero Galaxy

text: is an unbarred spiral galaxy.

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answers: 2: The answer has limited relevance and completeness, with significant gaps or inaccuracy.

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answers: galaxy

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answers: barred

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answers: unbarred

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answers: unbarred spiral galaxy

answers: NDQ_002603

answers: unbarred spiral

answers: NDQ_002604

answers: unbarred

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answers: unbarred

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answers: unbarred

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answers: Sombrero Galaxy

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answers: billions of stars

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answers: galaxy

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answers: spiral

answers: NDQ_002615

answers: galaxy

answers: NDQ_002617

answers: Sombrero

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: barred

answers: NDQ_002620

answers: spiral galaxy

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxy

answers: NDQ_002623

answers: Sombrero Galaxy

answers: NDQ_002624

answers: unbarred

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The Sombrero Galaxy is a spiral galaxy

answers: NDQ_002627

answers: The universe has billions of galaxies.

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: open star clusters

answers: NDQ_002630

answers: unbarred

answers: NDQ_002631

answers: unbarred spiral galaxy

answers: NDQ_002632

answers: dwarf galaxies

answers: NDQ_002633

answers: Sombrero Galaxy

answers: NDQ_002634

answers: The Sombrero Galaxy is an unbarred spiral galaxy

answers: NDQ_002635

answers: Our solar system orbits the central disk of our galaxy.

answers: NDQ_002636

answers: spiral galaxy

text: Finally the tidal radius, or Hill sphere, is the distance from the center of the globular cluster at which the external gravitation of the galaxy has more influence over the stars in the cluster than does the cluster itself. This is the distance at which the individual stars belonging to a cluster can be separated away by the galaxy. The tidal radius of M3 is about 40 arc minutes, or about 113 pc at the distance of 10.4 kpc.

text: Finally the tidal radius, or

text: Hill sphere

text: , is the distance from the center of the globular cluster at which the external gravitation of the galaxy has more influence over the stars in the cluster than does the cluster itself. This is the distance at which the individual stars belonging to a cluster can be separated away by the galaxy. The tidal radius of M3 is about 40 arc minutes, or about 113 pc at the distance of 10.4 kpc.

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answers: NDQ_002598

answers: globular cluster

answers: NDQ_002599

answers: individual stars

answers: NDQ_002600

answers: stars

answers: NDQ_002601

answers: Hill sphere

answers: NDQ_002602

answers: M3

answers: NDQ_002603

answers: external gravitation of the galaxy has more influence over the stars in the cluster

answers: NDQ_002604

answers: tidal radius

answers: NDQ_002605

answers: globular cluster

answers: NDQ_002606

answers: globular

answers: NDQ_002607

answers: tidal radius

answers: NDQ_002609

answers: 113 pc

answers: NDQ_002610

answers: globular cluster

answers: NDQ_002612

answers: globular

answers: NDQ_002615

answers: globular

answers: NDQ_002617

answers: globular

answers: NDQ_002618

answers: galaxy

answers: NDQ_002619

answers: cluster

answers: NDQ_002620

answers: globular cluster

answers: NDQ_002621

answers: a cluster

answers: NDQ_002622

answers: globular cluster

answers: NDQ_002623

answers: globular cluster

answers: NDQ_002624

answers: globular

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The tidal radius

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: globular cluster

answers: NDQ_002630

answers: globular cluster

answers: NDQ_002631

answers: Spiral

answers: NDQ_002632

answers: dwarf galaxies

answers: NDQ_002633

answers: 113 pc

answers: NDQ_002634

answers: galaxy

answers: NDQ_002635

answers: The tidal radius of M3

answers: NDQ_002636

answers: galaxy

text: In 1997, the Hubble telescope discovered a large number of intergalactic stars in the Virgo cluster of galaxies. Later in the 1990s scientists discovered another group of intergalactic stars in the Fornax cluster of galaxies.

text: In 1997, the

text: Hubble telescope

text: discovered a large number of intergalactic stars in the Virgo cluster of galaxies. Later in the 1990s scientists discovered another group of intergalactic stars in the

text: Fornax cluster

text: of galaxies.

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answers: 2: The answer has limited relevance and completeness, with significant gaps or inaccuracy.

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answers: NDQ_002598

answers: galaxies

answers: NDQ_002599

answers: large number

answers: NDQ_002600

answers: stars

answers: NDQ_002601

answers: galaxy

answers: NDQ_002602

answers: stars

answers: NDQ_002603

answers: stars

answers: NDQ_002604

answers: stars

answers: NDQ_002605

answers: galaxies

answers: NDQ_002606

answers: intergalactic

answers: NDQ_002607

answers: galaxies

answers: NDQ_002609

answers: billions of stars

answers: NDQ_002610

answers: galaxy

answers: NDQ_002612

answers: galaxy

answers: NDQ_002615

answers: Virgo cluster

answers: NDQ_002617

answers: Fornax

answers: NDQ_002618

answers: galaxy

answers: NDQ_002619

answers: cluster

answers: NDQ_002620

answers: galaxies

answers: NDQ_002621

answers: cluster

answers: NDQ_002622

answers: Virgo cluster

answers: NDQ_002623

answers: Fornax

answers: NDQ_002624

answers: Fornax

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: galaxies

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: open star clusters

answers: NDQ_002630

answers: cluster

answers: NDQ_002631

answers: Fornax

answers: NDQ_002632

answers: dwarf galaxies

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: Virgo

answers: NDQ_002635

answers: Our solar system orbits the central disk

answers: NDQ_002636

answers: galaxy

text: Ford built 200 lightweight Ford Galaxies for drag racing in 1963. All non-essential equipment was omitted. Modifications included fiberglass panels, aluminum bumpers, traction bars, and a competition-specification  engine factory rated at a conservative . This full-size car could run the quarter mile in a little over 12 seconds. Also built in 1963 were 5,000 road-legal versions that could be used as every day drivers (Ford claimed 0-60 in less than 6 seconds for the similarly powered 1966 Galaxie 500XL 427).

text: Ford built 200 lightweight Ford Galaxies for drag racing in 1963. All non-essential equipment was omitted. Modifications included fiberglass panels, aluminum bumpers, traction bars, and a competition-specification  engine factory rated at a conservative . This

text: full-size

text: car could run the quarter mile in a little over 12 seconds. Also built in 1963 were 5,000 road-legal versions that could be used as every day drivers (Ford claimed 0-60 in less than 6 seconds for the similarly powered 1966 Galaxie 500XL 427).

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answers: NDQ_002598

answers: Galaxies

answers: NDQ_002599

answers: 5,000

answers: NDQ_002600

answers: Galaxies

answers: NDQ_002601

answers: fiberglass panels

answers: NDQ_002602

answers: Galaxies

answers: NDQ_002603

answers: galaxies have very little gas

answers: NDQ_002604

answers: no

answers: NDQ_002605

answers: stars

answers: NDQ_002606

answers: lightweight

answers: NDQ_002607

answers: galaxies

answers: NDQ_002609

answers: 4.3 billion stars

answers: NDQ_002610

answers: galaxie

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answers: Galaxies

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answers: Galaxies

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answers: Galaxies

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answers: The Milky Way

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answers: Galaxies

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answers: Galaxies

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answers: Galaxie

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answers: Galaxies

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answers: Galaxies

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answers: Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is slowly spinning around our galaxy.

answers: NDQ_002627

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answers: Open star clusters

answers: NDQ_002630

answers: full-size

answers: NDQ_002631

answers: Spiral

answers: NDQ_002632

answers: Galaxies

answers: NDQ_002633

answers: Galaxies

answers: NDQ_002634

answers: Galaxies

answers: NDQ_002635

answers: Our solar system orbits the central disk of our galaxy

answers: NDQ_002636

answers: Galaxie

text: Stars and interstellar gas are bound by gravity to form galaxies, and groups of galaxies can be bound by gravity in galaxy clusters. With the exception of stars in the Milky Way and the galaxies in the Local Group, almost all galaxies are moving away from us due to the expansion of the universe.

text: Stars and interstellar gas are bound by gravity to form galaxies, and groups of galaxies can be bound by gravity in

text: galaxy clusters

text: . With the exception of stars in the

text: Milky Way

text: and the galaxies in the

text: Local Group

text: , almost all galaxies are moving away from us due to the

text: expansion of the universe

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answers: galaxy clusters

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answers: Local Group

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answers: Milky Way

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answers: Milky Way Galaxy

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answers: The Milky Way

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answers: Milky Way

answers: NDQ_002636

answers: Milky Way

text: Even though its mass is slightly larger than that of the Milky Way, the spiral will inevitably lose all its gas and dust as well as its chance of generating new stars later, and become a gas-poor galaxy with an old population of red stars. The finding sheds light on the process by which gas-rich galaxies might evolve into gas-poor galaxies over billions of years. The new observations also reveal one mechanism for forming of “homeless” stars seen scattered throughout galaxy clusters.

text: Even though its mass is slightly larger than that of the Milky Way, the spiral will inevitably lose all its gas and dust as well as its chance of generating new stars later, and become a gas-poor galaxy with an old population of red stars. The finding sheds light on the process by which gas-rich galaxies might evolve into gas-poor galaxies over billions of years. The new observations also reveal one mechanism for forming of “homeless” stars seen scattered throughout galaxy clusters.

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answers: NDQ_002602

answers: Milky Way

answers: NDQ_002603

answers: gas-poor galaxies

answers: NDQ_002604

answers: gas and dust

answers: NDQ_002605

answers: gas-poor

answers: NDQ_002606

answers: galaxy clusters

answers: NDQ_002607

answers: Galaxy clusters

answers: NDQ_002609

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answers: NDQ_002610

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answers: NDQ_002612

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answers: NDQ_002615

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answers: NDQ_002617

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answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

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answers: NDQ_002621

answers: galaxy clusters

answers: NDQ_002622

answers: galaxy clusters

answers: NDQ_002623

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answers: NDQ_002624

answers: Milky Way

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The Milky Way

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answers: NDQ_002631

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answers: NDQ_002632

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answers: NDQ_002633

answers: Galaxy clusters

answers: NDQ_002634

answers: Milky Way

answers: NDQ_002635

answers: Milky Way

answers: NDQ_002636

answers: Milky Way

text: A satellite galaxy is a galaxy that orbits a larger galaxy due to gravitational attraction. Although a galaxy is made of a large number of objects (such as stars, planets, and nebulae) that are not connected to each other, it has a center of mass, which represents a weighted average (by mass) of the positions of each component object.  This is similar to how an everyday object has a center of mass which is the weighted average of the positions of all its component atoms. Even within a satellite galaxy, the stars in turn orbit the galactic center.

text: A satellite galaxy is a galaxy that

text: orbit

text: s a larger galaxy due to

text: gravitational attraction

text: . Although a

text: galaxy

text: is made of a large number of objects (such as

text: star

text: s,

text: planet

text: s, and

text: nebula

text: e) that are not connected to each other, it has a

text: center of mass

text: , which represents a weighted average (by mass) of the positions of each component object.  This is similar to how an everyday object has a center of mass which is the weighted average of the positions of all its component

text: atom

text: s. Even within a satellite galaxy, the stars in turn orbit the galactic center.

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answers: NDQ_002598

answers: galaxy

answers: NDQ_002599

answers: a large number

answers: NDQ_002600

answers: stars

answers: NDQ_002601

answers: made of a large number of objects

answers: NDQ_002602

answers: satellite galaxy

answers: NDQ_002603

answers: gravitational attraction

answers: NDQ_002604

answers: stars in turn orbit the galactic center

answers: NDQ_002605

answers: not connected to each other

answers: NDQ_002606

answers: galaxy

answers: NDQ_002607

answers: nebulae

answers: NDQ_002609

answers: stars

answers: NDQ_002610

answers: center of mass

answers: NDQ_002612

answers: satellite galaxy

answers: NDQ_002615

answers: galaxy

answers: NDQ_002617

answers: satellite galaxy

answers: NDQ_002618

answers: galaxy

answers: NDQ_002619

answers: satellite galaxy

answers: NDQ_002620

answers: satellite galaxy

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxy

answers: NDQ_002623

answers: galaxy

answers: NDQ_002624

answers: satellite galaxy

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: orbits a larger galaxy

answers: NDQ_002627

answers: galaxy is made of a large number of objects

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: larger galaxy

answers: NDQ_002631

answers: elliptical

answers: NDQ_002632

answers: satellite galaxy

answers: NDQ_002633

answers: galaxy

answers: NDQ_002634

answers: galaxy

answers: NDQ_002635

answers: galaxy

answers: NDQ_002636

answers: galaxy

text: A common misconception is that kits were used for children. In fact, they were made for adults—their small size is so that they could be used in situations where a full-sized violin was too large to carry, or too expensive to own.  The "pocket fiddle" or "pochette" should not be confused with a saddle fiddle, the latter being a proper fiddle or violin with a nearly full-sized finger board, and a violin body that is the same shape as a full-sized version.

text: A common misconception is that kits were used for children. In fact, they were made for adults—their small size is so that they could be used in situations where a full-sized violin was too large to carry, or too expensive to own.  The "pocket fiddle" or "pochette" should not be confused with a saddle fiddle, the latter being a proper fiddle or violin with a nearly full-sized finger board, and a violin body that is the same shape as a full-sized version.

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answers: NDQ_002617

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answers: NDQ_002618

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answers: NDQ_002619

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answers: NDQ_002620

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answers: NDQ_002621

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answers: NDQ_002622

answers: full-sized

answers: NDQ_002623

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answers: NDQ_002624

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answers: NDQ_002625

answers: The "pocket fiddle" or "pochette" should not be confused with a saddle fiddle

answers: NDQ_002626

answers: The solar system revolves around our galaxy.

answers: NDQ_002627

answers: They were made for adults

answers: NDQ_002628

answers: Star clusters

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answers: NDQ_002631

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answers: dwarf galaxies are often found near larger galaxies

answers: NDQ_002633

answers: A common misconception is that kits were used for children

answers: NDQ_002634

answers: The solar system is within one of the spiral arms of our galaxy

answers: NDQ_002635

answers: orbits the central disk of our galaxy

answers: NDQ_002636

answers: The "pocket fiddle" or "pochette"

text: From 1959 to 1964, the Fairlane was a locally assembled version of the American Ford Fairlane which had taken its name from Henry Ford's estate, Fair Lane, near Dearborn, Michigan. This was Ford Australia's top-of-the-range model until replaced by an Australian-assembled version of the full-size American Ford Galaxie. In 1967, Ford Australia reintroduced the Fairlane, this time as an Australian-developed, luxury, long-wheelbase version of its mainstream Falcon, positioned between the Falcon and the Galaxie. The locally assembled Galaxie evolved into the LTD which was itself replaced in 1973 by an Australian-developed, Fairlane-based model, also known as the Ford LTD. In North America, unlike its designation in Australia, it was not considered a luxury vehicle. In Australia, "LTD" originally stood for "Lincoln Type Design", although Ford Australia later promoted a connection with the meaning "Limited".

text: From 1959 to 1964, the Fairlane was a locally assembled version of the American

text: Ford Fairlane

text: which had taken its name from

text: Henry Ford

text: 's estate,

text: Fair Lane

text: , near

text: Dearborn, Michigan

text: . This was Ford Australia's top-of-the-range model until replaced by an Australian-assembled version of the full-size American

text: Ford Galaxie

text: . In 1967, Ford Australia reintroduced the Fairlane, this time as an Australian-developed, luxury, long-wheelbase version of its mainstream

text: Falcon

text: , positioned between the Falcon and the Galaxie. The locally assembled Galaxie evolved into the

text: LTD

text: which was itself replaced in 1973 by an Australian-developed, Fairlane-based model, also known as the Ford LTD. In North America, unlike its designation in Australia, it was not considered a luxury vehicle. In Australia, "LTD" originally stood for "Lincoln Type Design", although Ford Australia later promoted a connection with the meaning "Limited".

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answers: galaxie

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: The locally assembled Galaxie

answers: NDQ_002628

answers: Star cluster

answers: NDQ_002629

answers: Open star cluster

answers: NDQ_002630

answers: full-size

answers: NDQ_002631

answers: Spiral

answers: NDQ_002632

answers: dwarf galaxie

answers: NDQ_002633

answers: galaxie

answers: NDQ_002634

answers: The local assembled Galaxie

answers: NDQ_002635

answers: orbits the central disk of our galaxy

answers: NDQ_002636

answers: Galaxie

text: H II regions are found only in spiral galaxies like the Milky Way and irregular galaxies. They are not seen in elliptical galaxies. In irregular galaxies, they may be dispersed throughout the galaxy, but in spirals they are most abundant within the spiral arms. A large spiral galaxy may contain thousands of H II regions.

text: H II regions are found only in

text: spiral galaxies

text: like the Milky Way and

text: irregular galaxies

text: . They are not seen in

text: elliptical galaxies

text: . In irregular galaxies, they may be dispersed throughout the galaxy, but in spirals they are most abundant within the spiral arms. A large spiral galaxy may contain thousands of H II regions.

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answers: they are most abundant within the spiral arms

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answers: NDQ_002624

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answers: NDQ_002625

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answers: NDQ_002634

answers: 4

answers: NDQ_002635

answers: 0

answers: NDQ_002636

answers: 4

answers: NDQ_002598

answers: H II regions

answers: NDQ_002599

answers: thousands

answers: NDQ_002600

answers: H II regions

answers: NDQ_002601

answers: spiral arms

answers: NDQ_002602

answers: Milky Way and irregular galaxies

answers: NDQ_002603

answers: H II regions

answers: NDQ_002604

answers: H II regions

answers: NDQ_002605

answers: H II regions

answers: NDQ_002606

answers: irregular galaxies

answers: NDQ_002607

answers: A large spiral galaxy may contain thousands of H II regions

answers: NDQ_002609

answers: thousands

answers: NDQ_002610

answers: Milky Way

answers: NDQ_002612

answers: spiral

answers: NDQ_002615

answers: H II regions

answers: NDQ_002617

answers: Ellipstical

answers: NDQ_002618

answers: H II regions

answers: NDQ_002619

answers: H II regions

answers: NDQ_002620

answers: Milky Way

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: H II regions

answers: NDQ_002623

answers: H II regions are found only in spiral galaxies

answers: NDQ_002624

answers: Milky Way

answers: NDQ_002625

answers: Milky Way

answers: NDQ_002626

answers: The Milky Way

answers: NDQ_002627

answers: The Milky Way

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: large spiral galaxy

answers: NDQ_002631

answers: Spiral galaxies

answers: NDQ_002632

answers: Dwarf galaxies

answers: NDQ_002633

answers: The Milky Way

answers: NDQ_002634

answers: Milky Way

answers: NDQ_002635

answers: Milky Way

answers: NDQ_002636

answers: Milky Way

text: In the updated Hubble sequence galaxy morphological classification scheme by the French astronomer Gérard de Vaucouleurs in 1959, NGC 4889 is classified as an E4 type galaxy, which means it has a flat distribution of stars within its width. It is also classified as a cD galaxy, a giant type of D galaxy, a classification devised by the American astronomer William Wilson Morgan in 1958 for galaxies with an elliptical-shaped nucleus surrounded by an immense, diffuse, dustless, extended halo.

text: In the updated

text: Hubble sequence

text: galaxy morphological classification

text: scheme by the French astronomer

text: Gérard de Vaucouleurs

text: in 1959, NGC 4889 is classified as an E4 type galaxy, which means it has a flat distribution of stars within its width. It is also classified as a cD galaxy, a giant type of D galaxy, a classification devised by the

text: American

text: astronomer

text: William Wilson Morgan

text: in 1958 for galaxies with an elliptical-shaped nucleus surrounded by an immense, diffuse, dustless, extended halo.

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answers: NDQ_002634

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answers: NDQ_002635

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answers: NDQ_002636

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answers: NDQ_002598

answers: flat distribution of stars

answers: NDQ_002599

answers: stars

answers: NDQ_002600

answers: stars

answers: NDQ_002601

answers: elliptical-shaped

answers: NDQ_002602

answers: galaxies with an elliptical-shaped nucleus

answers: NDQ_002603

answers: dustless

answers: NDQ_002604

answers: halo

answers: NDQ_002605

answers: flat distribution

answers: NDQ_002606

answers: morphological

answers: NDQ_002607

answers: NGC 4889

answers: NDQ_002609

answers: stars

answers: NDQ_002610

answers: cD galaxy

answers: NDQ_002612

answers: D galaxy

answers: NDQ_002615

answers: NGC 4889

answers: NDQ_002617

answers: cD galaxy

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: halo

answers: NDQ_002620

answers: E4 type galaxy

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: immense

answers: NDQ_002623

answers: It is also classified as a cD galaxy

answers: NDQ_002624

answers: D galaxy

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The solar system is rotating around our galaxy.

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: open star clusters

answers: NDQ_002630

answers: immense

answers: NDQ_002631

answers: It is also classified as a giant type of D galaxy

answers: NDQ_002632

answers: NGC 4889

answers: NDQ_002633

answers: galaxies

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answers: galaxy

answers: NDQ_002635

answers: galaxy

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answers: elliptical

text: The reason H II regions rarely appear in elliptical galaxies is that ellipticals are believed to form through galaxy mergers. In galaxy clusters, such mergers are frequent. When galaxies collide, individual stars almost never collide, but the GMCs and H II regions in the colliding galaxies are severely agitated. Under these conditions, enormous bursts of star formation are triggered, so rapid that most of the gas is converted into stars rather than the normal rate of 10% or less.

text: The reason H II regions rarely appear in elliptical galaxies is that ellipticals are believed to form through galaxy mergers. In

text: galaxy cluster

text: s, such mergers are frequent. When galaxies collide, individual stars almost never collide, but the GMCs and H II regions in the colliding galaxies are severely agitated. Under these conditions, enormous bursts of star formation are triggered, so rapid that most of the gas is converted into stars rather than the normal rate of 10% or less.

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answers: NDQ_002598

answers: galaxy clusters

answers: NDQ_002599

answers: 10% or less

answers: NDQ_002600

answers: H II regions

answers: NDQ_002601

answers: galaxy mergers

answers: NDQ_002602

answers: galaxy clusters

answers: NDQ_002603

answers: galaxy mergers

answers: NDQ_002604

answers: galaxy clusters

answers: NDQ_002605

answers: gas

answers: NDQ_002606

answers: galaxies

answers: NDQ_002607

answers: galaxy clusters

answers: NDQ_002609

answers: 10 billion stars

answers: NDQ_002610

answers: galaxy clusters

answers: NDQ_002612

answers: galaxy clusters

answers: NDQ_002615

answers: galaxy clusters

answers: NDQ_002617

answers: elliptical

answers: NDQ_002618

answers: galaxy clusters

answers: NDQ_002619

answers: GMCs

answers: NDQ_002620

answers: galaxy clusters

answers: NDQ_002621

answers: galaxy clusters

answers: NDQ_002622

answers: galaxy clusters

answers: NDQ_002623

answers: galaxies collide

answers: NDQ_002624

answers: galaxy clusters

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: It is rotating around our galaxy.

answers: NDQ_002627

answers: galaxy clusters

answers: NDQ_002628

answers: galaxy clusters

answers: NDQ_002629

answers: open star clusters

answers: NDQ_002630

answers: galaxy clusters

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answers: spiral galaxies

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answers: galaxy clusters

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answers: galaxy clusters

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answers: galaxy clusters

answers: NDQ_002635

answers: galaxy

answers: NDQ_002636

answers: galaxy clusters

text: The final images were released at a meeting of the American Astronomical Society in January 1996, and revealed a plethora of distant, faint galaxies. About 3,000 distinct galaxies could be identified in the images, with both irregular and spiral galaxies clearly visible, although some galaxies in the field are only a few pixels across. In all, the HDF is thought to contain fewer than twenty galactic foreground stars; by far the majority of objects in the field are distant galaxies.

text: The final images were released at a meeting of the

text: American Astronomical Society

text: in January 1996, and revealed a plethora of distant, faint galaxies. About 3,000 distinct galaxies could be identified in the images, with both

text: irregular

text: and

text: spiral galaxies

text: clearly visible, although some galaxies in the field are only a few pixels across. In all, the HDF is thought to contain fewer than twenty galactic foreground stars; by far the majority of objects in the field are distant galaxies.

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answers: galaxies

answers: NDQ_002599

answers: twenty

answers: NDQ_002600

answers: stars

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answers: galaxy are only a few pixels across

answers: NDQ_002602

answers: irregular and spiral

answers: NDQ_002603

answers: distant

answers: NDQ_002604

answers: stars

answers: NDQ_002605

answers: distant galaxies

answers: NDQ_002606

answers: irregular

answers: NDQ_002607

answers: galaxies

answers: NDQ_002609

answers: twenty galactic foreground stars

answers: NDQ_002610

answers: galaxy

answers: NDQ_002612

answers: spiral

answers: NDQ_002615

answers: galaxies

answers: NDQ_002617

answers: irregular

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: HDF

answers: NDQ_002620

answers: distant galaxies

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxies

answers: NDQ_002623

answers: galaxies

answers: NDQ_002624

answers: HDF

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Galaxies

answers: NDQ_002627

answers: About 3,000 distinct galaxies

answers: NDQ_002628

answers: star clusters

answers: NDQ_002629

answers: globular star clusters

answers: NDQ_002630

answers: galaxies

answers: NDQ_002631

answers: spiral galaxies

answers: NDQ_002632

answers: distant, faint galaxies

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: galaxy

answers: NDQ_002635

answers: Our solar system orbits

answers: NDQ_002636

answers: galaxies

text: Although it appears that globular clusters contain some of the first stars to be produced in the galaxy, their origins and their role in galactic evolution are still unclear. It does appear clear that globular clusters are significantly different from dwarf elliptical galaxies and were formed as part of the star formation of the parent galaxy rather than as a separate galaxy.

text: Although it appears that globular clusters contain some of the first stars to be produced in the galaxy, their

text: origins

text: and their role in galactic evolution are still unclear. It does appear clear that globular clusters are significantly different from

text: dwarf elliptical galaxies

text: and were formed as part of the star formation of the parent galaxy rather than as a separate galaxy.

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answers: NDQ_002598

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answers: NDQ_002602

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answers: NDQ_002605

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answers: NDQ_002606

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answers: NDQ_002607

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answers: NDQ_002609

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answers: 2

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answers: NDQ_002620

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answers: NDQ_002621

answers: 4

answers: NDQ_002622

answers: 4

answers: NDQ_002623

answers: 3

answers: NDQ_002624

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answers: NDQ_002625

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answers: NDQ_002626

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answers: NDQ_002627

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answers: 3

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answers: 4

answers: NDQ_002634

answers: 0

answers: NDQ_002635

answers: 0

answers: NDQ_002636

answers: 4

answers: NDQ_002598

answers: globular clusters

answers: NDQ_002599

answers: galaxy

answers: NDQ_002600

answers: stars

answers: NDQ_002601

answers: dwarf elliptical

answers: NDQ_002602

answers: dwarf elliptical

answers: NDQ_002603

answers: gas and dust

answers: NDQ_002604

answers: galaxies

answers: NDQ_002605

answers: galaxies

answers: NDQ_002606

answers: unclear

answers: NDQ_002607

answers: are significantly different from dwarf elliptical galaxies

answers: NDQ_002609

answers: billions of stars

answers: NDQ_002610

answers: galaxy

answers: NDQ_002612

answers: elliptical

answers: NDQ_002615

answers: globular clusters

answers: NDQ_002617

answers: dwarf elliptical

answers: NDQ_002618

answers: galaxy

answers: NDQ_002619

answers: globular clusters

answers: NDQ_002620

answers: globular clusters

answers: NDQ_002621

answers: clusters

answers: NDQ_002622

answers: globular clusters

answers: NDQ_002623

answers: globular clusters

answers: NDQ_002624

answers: dwarf

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The solar system is rotating around our galaxy.

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: globular clusters

answers: NDQ_002630

answers: dwarf elliptical

answers: NDQ_002631

answers: It does appear clear that globular clusters are significantly different

answers: NDQ_002632

answers: dwarf elliptical galaxies

answers: NDQ_002633

answers: globular clusters

answers: NDQ_002634

answers: galaxy

answers: NDQ_002635

answers: galaxy

answers: NDQ_002636

answers: galaxy

text: Examples of irregular galaxies: M82, NGC 1427A, Large Magellanic Cloud, Small Magellanic Cloud.

text: Examples of irregular galaxies:

text: NGC 1427A

text: Large Magellanic Cloud

text: Small Magellanic Cloud

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answers: 3: The answer has limited relevance and completeness, with noticeable gaps or inaccuracy.

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answers: NDQ_002598

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answers: NDQ_002604

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answers: NDQ_002605

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answers: NDQ_002606

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answers: NDQ_002634

answers: 0

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answers: 2

answers: NDQ_002598

answers: star clusters

answers: NDQ_002599

answers: galaxies

answers: NDQ_002600

answers: galaxies

answers: NDQ_002601

answers: Magellanic Cloud

answers: NDQ_002602

answers: irregular

answers: NDQ_002603

answers: irregular galaxies

answers: NDQ_002604

answers: irregular galaxy

answers: NDQ_002605

answers: galaxies

answers: NDQ_002606

answers: irregular galaxies

answers: NDQ_002607

answers: irregular galaxies

answers: NDQ_002609

answers: 3 billion stars

answers: NDQ_002610

answers: Magellanic Cloud

answers: NDQ_002612

answers: irregular

answers: NDQ_002615

answers: galaxies

answers: NDQ_002617

answers: Large Magellanic Cloud

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: Small Magellanic Cloud

answers: NDQ_002620

answers: Large Magellanic Cloud

answers: NDQ_002621

answers: galaxies

answers: NDQ_002622

answers: galaxies

answers: NDQ_002623

answers: Elliptical galaxies

answers: NDQ_002624

answers: irregular

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: galaxies

answers: NDQ_002628

answers: Star clusters

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: Large Magellanic Cloud

answers: NDQ_002631

answers: irregular galaxies

answers: NDQ_002632

answers: Small Magellanic Cloud

answers: NDQ_002633

answers: Large Magellanic Cloud

answers: NDQ_002634

answers: Our solar system is within one of the spiral arms

answers: NDQ_002635

answers: Our solar system orbits the central disk

answers: NDQ_002636

answers: irregular galaxies

text: Other notable spiral galaxies in Canes Venatici are the Sunflower Galaxy (M63, NGC 5055), M94 (NGC 4736), and M106 (NGC 4258). M63, the Sunflower Galaxy, was named for its appearance in large amateur telescopes. It is a spiral galaxy with an integrated magnitude of 9.0. M94 is a small face-on spiral galaxy with an approximate magnitude of 8.0, about 15 million light-years from Earth. NGC 4631 is a barred spiral galaxy, which is one of the largest and brightest edge-on galaxies in the sky.

text: Other notable spiral galaxies in Canes Venatici are the

text: Sunflower Galaxy

text: (M63, NGC 5055),

text: (NGC 4736), and

text: (NGC 4258). M63, the Sunflower Galaxy, was named for its appearance in large amateur telescopes. It is a spiral galaxy with an integrated magnitude of 9.0. M94 is a small face-on spiral galaxy with an approximate magnitude of 8.0, about 15 million light-years from Earth.

text: NGC 4631

text: is a barred spiral galaxy, which is one of the largest and brightest edge-on galaxies in the sky.

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answers: the Sunflower Galaxy

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answers: magnitude of 9.0

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answers: face-on

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answers: NDQ_002609

answers: 1.5 billion stars

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text: The result of N-body simulations suggests that the universe is composed largely of voids, whose densities might be as low as one tenth the cosmological mean. The matter condenses in large filaments and haloes which have an intricate web-like structure. These form galaxy groups, clusters and superclusters. While the simulations appear to agree broadly with observations, their interpretation is complicated by the understanding of how dense accumulations of dark matter spur galaxy formation. In particular, many more small haloes form than we see in astronomical observations as dwarf galaxies and globular clusters. This is known as the galaxy bias problem, and a variety of explanations have been proposed. Most account for it as an effect in the complicated physics of galaxy formation, but some have suggested that it is a problem with our model of dark matter and that some effect, such as warm dark matter, prevents the formation of the smallest haloes.

text: The result of N-body simulations suggests that the universe is composed largely of

text: void

text: s, whose densities might be as low as one tenth the cosmological mean. The matter condenses in large

text: filament

text: s and

text: halo

text: es which have an intricate web-like structure. These form

text: galaxy

text: groups, clusters

text: and

text: supercluster

text: s. While the simulations appear to agree broadly with observations, their interpretation is complicated by the understanding of how dense accumulations of dark matter spur galaxy formation. In particular, many more small haloes form than we see in astronomical observations as

text: dwarf galaxies

text: and

text: globular cluster

text: s. This is known as the

text: galaxy bias

text: problem, and a variety of explanations have been proposed. Most account for it as an effect in the complicated physics of galaxy formation, but some have suggested that it is a problem with our model of

text: dark matter

text: and that some effect, such as

text: warm dark matter

text: , prevents the formation of the smallest haloes.

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answers: globular clusters

answers: NDQ_002599

answers: many more small haloes

answers: NDQ_002600

answers: dark matter

answers: NDQ_002601

answers: web-like structure

answers: NDQ_002602

answers: dwarf galaxies

answers: NDQ_002603

answers: voids

answers: NDQ_002604

answers: intricate web-like structure

answers: NDQ_002605

answers: voids

answers: NDQ_002606

answers: voids

answers: NDQ_002607

answers: dwarf galaxies

answers: NDQ_002609

answers: one tenth

answers: NDQ_002610

answers: warm dark matter

answers: NDQ_002612

answers: dwarf galaxies

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answers: globular cluster

answers: NDQ_002617

answers: globular cluster

answers: NDQ_002618

answers: The result of N-body simulations

answers: NDQ_002619

answers: halo

answers: NDQ_002620

answers: globular clusters

answers: NDQ_002621

answers: clusters

answers: NDQ_002622

answers: superclusters

answers: NDQ_002623

answers: globular clusters

answers: NDQ_002624

answers: dwarf

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The result of N-body simulations

answers: NDQ_002627

answers: galaxy groups, clusters and superclusters

answers: NDQ_002628

answers: clusters

answers: NDQ_002629

answers: open star clusters

answers: NDQ_002630

answers: dwarf galaxies

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answers: spiral galaxies

answers: NDQ_002632

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answers: galaxy groups, clusters and superclusters

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answers: galaxy groups

answers: NDQ_002635

answers: galaxy

answers: NDQ_002636

answers: web-like structure

text: The Milky Way galaxy falls within the Local Group, which is a poor and irregular cluster of galaxies. Poor clusters may contain only a few dozen galaxies, as compared to rich clusters with hundreds or even thousands. The Local Group is near the Local Supercluster (also known as the Virgo Supercluster), which has a diameter of 100 million light-years. The Local Supercluster contains a total of about 10 times the mass of the Sun.

text: The Milky Way galaxy falls within the Local Group, which is a poor and irregular cluster of galaxies. Poor clusters may contain only a few dozen galaxies, as compared to rich clusters with hundreds or even thousands. The Local Group is near the Local Supercluster (also known as the

text: Virgo Supercluster

text: ), which has a diameter of 100 million light-years. The Local Supercluster contains a total of about 10 times the mass of the Sun.

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answers: NDQ_002598

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answers: NDQ_002605

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answers: NDQ_002606

answers: 3

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answers: 4

answers: NDQ_002610

answers: 0

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answers: 4

answers: NDQ_002617

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answers: 0

answers: NDQ_002620

answers: 3

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answers: 4

answers: NDQ_002622

answers: 5

answers: NDQ_002623

answers: 0

answers: NDQ_002624

answers: 0

answers: NDQ_002625

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answers: NDQ_002626

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answers: NDQ_002627

answers: 4

answers: NDQ_002628

answers: 4

answers: NDQ_002629

answers: 3

answers: NDQ_002630

answers: 4

answers: NDQ_002631

answers: 2

answers: NDQ_002632

answers: 2

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answers: 4

answers: NDQ_002634

answers: 4

answers: NDQ_002635

answers: 0

answers: NDQ_002636

answers: 4

answers: NDQ_002598

answers: rich clusters with hundreds or even thousands

answers: NDQ_002599

answers: thousands

answers: NDQ_002600

answers: galaxies

answers: NDQ_002601

answers: may contain only a few dozen galaxies

answers: NDQ_002602

answers: rich clusters

answers: NDQ_002603

answers: poor and irregular cluster of galaxies

answers: NDQ_002604

answers: galaxies

answers: NDQ_002605

answers: galaxies

answers: NDQ_002606

answers: irregular

answers: NDQ_002607

answers: Rich clusters with hundreds or even thousands

answers: NDQ_002609

answers: 10 times the mass of the Sun

answers: NDQ_002610

answers: Local Supercluster

answers: NDQ_002612

answers: Milky Way galaxy

answers: NDQ_002615

answers: rich

answers: NDQ_002617

answers: The Milky Way galaxy

answers: NDQ_002618

answers: The Milky Way galaxy

answers: NDQ_002619

answers: cluster

answers: NDQ_002620

answers: poor and irregular cluster of galaxies

answers: NDQ_002621

answers: cluster

answers: NDQ_002622

answers: rich

answers: NDQ_002623

answers: The Milky Way galaxy

answers: NDQ_002624

answers: Milky Way galaxy

answers: NDQ_002625

answers: The Milky Way galaxy

answers: NDQ_002626

answers: The Milky Way galaxy

answers: NDQ_002627

answers: The Milky Way galaxy

answers: NDQ_002628

answers: galaxies

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: rich clusters

answers: NDQ_002631

answers: The Milky Way galaxy

answers: NDQ_002632

answers: The Local Group is near the Local Supercluster

answers: NDQ_002633

answers: The Local Supercluster

answers: NDQ_002634

answers: Local Supercluster

answers: NDQ_002635

answers: The Milky Way galaxy

answers: NDQ_002636

answers: The Milky Way galaxy

text: Examples of elliptical galaxies: M49, M59, M60, M87, NGC 4125.

text: Examples of elliptical galaxies:

text: NGC 4125

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answers: 3: The answer has limited relevance and completeness, with noticeable gaps or inaccuracy.

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answers: 0

answers: NDQ_002598

answers: 0

answers: NDQ_002599

answers: 0

answers: NDQ_002600

answers: 0

answers: NDQ_002601

answers: 0

answers: NDQ_002602

answers: 4

answers: NDQ_002603

answers: 0

answers: NDQ_002604

answers: 0

answers: NDQ_002605

answers: 0

answers: NDQ_002606

answers: 4

answers: NDQ_002607

answers: 1

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answers: 0

answers: NDQ_002610

answers: 0

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answers: 4

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answers: 0

answers: NDQ_002617

answers: 5

answers: NDQ_002618

answers: 0

answers: NDQ_002619

answers: 0

answers: NDQ_002620

answers: 2

answers: NDQ_002621

answers: 4

answers: NDQ_002622

answers: 0

answers: NDQ_002623

answers: 0

answers: NDQ_002624

answers: 0

answers: NDQ_002625

answers: 0

answers: NDQ_002626

answers: 0

answers: NDQ_002627

answers: 4

answers: NDQ_002628

answers: 3

answers: NDQ_002629

answers: 3

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answers: 4

answers: NDQ_002631

answers: 2

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answers: 2

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answers: 0

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answers: 0

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answers: 0

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answers: 1

answers: NDQ_002598

answers: galaxies

answers: NDQ_002599

answers: stars

answers: NDQ_002600

answers: stars

answers: NDQ_002601

answers: elliptical

answers: NDQ_002602

answers: elliptical

answers: NDQ_002603

answers: elliptical galaxies have very little gas and dust

answers: NDQ_002604

answers: elliptical

answers: NDQ_002605

answers: galaxies

answers: NDQ_002606

answers: elliptical

answers: NDQ_002607

answers: elliptical

answers: NDQ_002609

answers: 4.3 billion stars

answers: NDQ_002610

answers: galaxy

answers: NDQ_002612

answers: Elliptical

answers: NDQ_002615

answers: galaxies

answers: NDQ_002617

answers: elliptical

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: M60

answers: NDQ_002620

answers: elliptical

answers: NDQ_002621

answers: galaxies

answers: NDQ_002622

answers: Galaxies

answers: NDQ_002623

answers: It's impossible to say

answers: NDQ_002624

answers: elliptical

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is rotating around our galaxy.

answers: NDQ_002627

answers: galaxies

answers: NDQ_002628

answers: A star cluster

answers: NDQ_002629

answers: globular star clusters

answers: NDQ_002630

answers: elliptical

answers: NDQ_002631

answers: Spiral

answers: NDQ_002632

answers: Dwarf galaxies

answers: NDQ_002633

answers: elliptical galaxies

answers: NDQ_002634

answers: elliptical galaxies

answers: NDQ_002635

answers: Our solar system orbits the central disk of our galaxy

answers: NDQ_002636

answers: elliptical

text: A low-mass X-ray binary (LMXB) is a binary star system where one of the components is either a black hole or neutron star.  The other component, a donor, usually fills its Roche lobe and therefore transfers mass to the compact star.  The donor is less massive than the compact object, and can be on the main sequence, a degenerate dwarf (white dwarf), or an evolved star (red giant).  Approximately two hundred LMXBs have been detected in the Milky Way, and of these, thirteen LMXBs have been discovered in globular clusters.  The Chandra X-ray Observatory has revealed LMXBs in many distant galaxies.

text: A low-mass X-ray binary (LMXB) is a

text: binary star

text: system where one of the components is either a

text: black hole

text: or

text: neutron star

text: .  The other component, a donor, usually fills its

text: Roche lobe

text: and therefore transfers mass to the compact star.  The donor is less massive than the compact object, and can be on the

text: main sequence

text: , a degenerate dwarf (

text: white dwarf

text: ), or an evolved star (

text: red giant

text: ).  Approximately two hundred LMXBs have been detected in the

text: Milky Way

text: , and of these, thirteen LMXBs have been discovered in

text: globular cluster

text: s.  The

text: Chandra X-ray Observatory

text: has revealed LMXBs in many distant galaxies.

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answers: NDQ_002609

answers: 4

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answers: 4

answers: NDQ_002621

answers: 0

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answers: NDQ_002624

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answers: NDQ_002625

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answers: globular clusters

answers: NDQ_002599

answers: Approximately two hundred

answers: NDQ_002600

answers: globular clusters

answers: NDQ_002601

answers: Roche lobe

answers: NDQ_002602

answers: Milky Way

answers: NDQ_002603

answers: black hole or neutron star

answers: NDQ_002604

answers: lobe

answers: NDQ_002605

answers: neutron star

answers: NDQ_002606

answers: globular

answers: NDQ_002607

answers: LMXBs have been discovered in globular clusters

answers: NDQ_002609

answers: two hundred

answers: NDQ_002610

answers: black hole

answers: NDQ_002612

answers: Milky Way

answers: NDQ_002615

answers: globular cluster

answers: NDQ_002617

answers: Milky Way

answers: NDQ_002618

answers: X-ray

answers: NDQ_002619

answers: globular cluster

answers: NDQ_002620

answers: Milky Way

answers: NDQ_002621

answers: Galaxies

answers: NDQ_002622

answers: globular cluster

answers: NDQ_002623

answers: globular clusters

answers: NDQ_002624

answers: globular

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The other component, a donor

answers: NDQ_002627

answers: The Milky Way

answers: NDQ_002628

answers: globular cluster

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: globular clusters

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answers: spiral

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answers: globular clusters

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answers: galaxies

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answers: Milky Way

answers: NDQ_002635

answers: Milky Way

answers: NDQ_002636

answers: Milky Way

text: The rate of star formation in the Milky Way is much higher, with Andromeda Galaxy producing only about one solar mass per year compared to 3–5 solar masses for the Milky Way. The rate of supernovae in the Milky Way is also double that of Andromeda Galaxy. This suggests that the latter once experienced a great star formation phase, but is now in a relative state of quiescence, whereas the Milky Way is experiencing more active star formation. Should this continue, the luminosity in the Milky Way may eventually overtake that of Andromeda Galaxy.

text: The rate of star formation in the Milky Way is much higher, with Andromeda Galaxy producing only about one solar mass per year compared to 3–5 solar masses for the Milky Way. The rate of

text: supernova

text: e in the Milky Way is also double that of Andromeda Galaxy. This suggests that the latter once experienced a great star formation phase, but is now in a relative state of quiescence, whereas the Milky Way is experiencing more active star formation. Should this continue, the luminosity in the Milky Way may eventually overtake that of Andromeda Galaxy.

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answers: NDQ_002604

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answers: NDQ_002605

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answers: NDQ_002606

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answers: NDQ_002607

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answers: NDQ_002609

answers: 5

answers: NDQ_002610

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answers: NDQ_002612

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answers: NDQ_002617

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answers: NDQ_002618

answers: 4

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answers: NDQ_002620

answers: 3

answers: NDQ_002621

answers: 5

answers: NDQ_002622

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answers: NDQ_002623

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answers: NDQ_002625

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answers: NDQ_002626

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answers: NDQ_002627

answers: 4

answers: NDQ_002628

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answers: NDQ_002634

answers: 4

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answers: NDQ_002636

answers: 4

answers: NDQ_002598

answers: supernovae

answers: NDQ_002599

answers: galaxy

answers: NDQ_002600

answers: stars

answers: NDQ_002601

answers: the Milky Way

answers: NDQ_002602

answers: Milky Way

answers: NDQ_002603

answers: Andromeda Galaxy

answers: NDQ_002604

answers: star formation

answers: NDQ_002605

answers: active

answers: NDQ_002606

answers: Galaxy

answers: NDQ_002607

answers: Andromeda Galaxy

answers: NDQ_002609

answers: 5 solar masses

answers: NDQ_002610

answers: Milky Way

answers: NDQ_002612

answers: Milky Way

answers: NDQ_002615

answers: Milky Way

answers: NDQ_002617

answers: Milky Way

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: galaxy

answers: NDQ_002620

answers: Milky Way

answers: NDQ_002621

answers: Galaxy

answers: NDQ_002622

answers: Milky Way

answers: NDQ_002623

answers: Andromeda Galaxy

answers: NDQ_002624

answers: Milky Way

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: The Milky Way Galaxy

answers: NDQ_002628

answers: Milky Way

answers: NDQ_002629

answers: Open star clusters contain more stars

answers: NDQ_002630

answers: Milky Way

answers: NDQ_002631

answers: Andromeda Galaxy

answers: NDQ_002632

answers: Andromeda Galaxy

answers: NDQ_002633

answers: The Milky Way

answers: NDQ_002634

answers: Milky Way

answers: NDQ_002635

answers: The Milky Way

answers: NDQ_002636

answers: Milky Way

text: Our own galaxy, the Milky Way, is a large disk-shaped barred-spiral galaxy about 30 kiloparsecs in diameter and a kiloparsec thick. It contains about two hundred billion (2×10) stars and has a total mass of about six hundred billion (6×10) times the mass of the Sun.

text: Our own galaxy, the

text: Milky Way

text: , is a large disk-shaped barred-spiral galaxy about 30 kiloparsecs in diameter and a kiloparsec thick. It contains about two hundred billion (2×10) stars and has a total mass of about six hundred billion (6×10) times the mass of the Sun.

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text: Notable galaxy clusters in the relatively nearby Universe include the Virgo Cluster, Fornax Cluster, Hercules Cluster, and the Coma Cluster. A very large aggregation of galaxies known as the Great Attractor, dominated by the Norma Cluster, is massive enough to affect the local expansion of the Universe. Notable galaxy clusters in the distant, high-redshift Universe include SPT-CL J0546-5345 and SPT-CL J2106-5844, the most massive galaxy clusters found in the early Universe. In the last few decades, they are also found to be relevant sites of particle acceleration, a feature that has been discovered by observing non-thermal diffuse radio emissions, such as radio halos and radio relics. Using the Chandra X-ray Observatory, structures such as cold fronts and shock waves have also been found in many galaxy clusters.

text: Notable galaxy clusters in the relatively nearby Universe include the

text: Virgo Cluster

text: Fornax Cluster

text: Hercules Cluster

text: , and the

text: Coma Cluster

text: . A very large aggregation of galaxies known as the

text: Great Attractor

text: , dominated by the

text: Norma Cluster

text: , is massive enough to affect the

text: local expansion of the Universe

text: . Notable galaxy clusters in the distant, high-redshift Universe include

text: SPT-CL J0546-5345

text: and

text: SPT-CL J2106-5844

text: , the most massive galaxy clusters found in the early Universe. In the last few decades, they are also found to be relevant sites of particle acceleration, a feature that has been discovered by observing non-thermal diffuse radio emissions, such as

text: radio halo

text: s and

text: radio relics

text: . Using the

text: Chandra X-ray Observatory

text: , structures such as cold fronts and

text: shock waves

text: have also been found in many galaxy clusters.

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text: She also grew to hate Fifth for his actions, seeing him as nothing more than a weakling which also resulted in her becoming a major adversary in the eighth season of the series, threatening the entire Milky Way galaxy and its people.

text: She also grew to hate Fifth for his actions, seeing him as nothing more than a weakling which also resulted in her becoming a major adversary in the eighth season of the series, threatening the entire Milky Way galaxy and its people.

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text: The Large Magellanic Cloud is usually considered an irregular galaxy. However, it shows signs of a bar structure, and is often reclassified as a Magellanic-type dwarf spiral galaxy.

text: The Large Magellanic Cloud is usually considered an

text: irregular galaxy

text: . However, it shows signs of a bar structure, and is often reclassified as a

text: Magellanic-type

text: dwarf spiral galaxy

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text: Samsung Galaxy A8 refers to two Samsung Galaxy Android smart phones released in 2015 and 216.

text: Samsung Galaxy A8 refers to two

text: Samsung Galaxy

text: Android

text: smart phones

text: released in 2015 and 216.

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text: DDO 69 (also known as Leo A, Leo III, PGC 28868 or UGC 5364) is an irregular galaxy which is located in the constellation of Leo. It is a small satellite galaxy of our galaxy, the Milky Way.

text: DDO 69

text: (also known as

text: Leo

text: A,

text: Leo

text: III,

text: PGC

text: 28868 or

text: UGC

text: 5364) is an

text: irregular galaxy

text: which is located in the

text: constellation

text: of

text: Leo

text: . It is a small

text: satellite galaxy

text: of our

text: galaxy

text: the Milky Way

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text: One of the original aims for Galaxy Zoo was to explore which way galaxies rotated. Cosmologist Kate Land stated: "Some people have argued that galaxies are rotating all in agreement with each other, not randomly as we'd expect. We want people to classify the galaxies according to which way they're rotating and I'll be able to go and see if there's anything bizarre going on. If there are any patterns that we're not expecting, it could really turn up some surprises." In Galaxy Zoo 1, volunteers were asked to judge from the SDSS images whether the galaxies were elliptical or spiral and, if spiral, whether they were rotating in a clockwise or anti-clockwise direction. The rotation, also called the Chirality, of galaxies has been examined in several Galaxy Zoo related papers.

text: One of the original aims for Galaxy Zoo was to explore which way galaxies rotated. Cosmologist Kate Land stated: "Some people have argued that galaxies are rotating all in agreement with each other, not randomly as we'd expect. We want people to classify the galaxies according to which way they're rotating and I'll be able to go and see if there's anything bizarre going on. If there are any patterns that we're not expecting, it could really turn up some surprises." In Galaxy Zoo 1, volunteers were asked to judge from the

text: SDSS

text: images whether the galaxies were

text: elliptical

text: or

text: spiral

text: and, if spiral, whether they were rotating in a

text: clockwise

text: or

text: anti-clockwise

text: direction. The rotation, also called the

text: Chirality

text: , of galaxies has been examined in several Galaxy Zoo related papers.

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answers: It could really turn up some surprises

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answers: Galaxy Zoo

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text: The stream covers over 100 square degrees, and possibly as much as 1,000 square degrees (approximately 5% of the hemisphere visible at any one time, or 5,000 times the area of the full moon).  Despite its proximity to the solar system and the solid angle that it consequently covers, the stream contains only a few hundred thousand stars.  The low surface brightness of the galaxy (possibly as low as 32.5 mag/arcmin²) may have militated against its detection in surveys before SDSS.  The number of stars in the stream is not greatly in excess of a star cluster, and it has been described by a member of the team that discovered it as "a rather pathetic galaxy", in comparison to the Milky Way.  Many of the stars have been known for centuries and thought of as normal Milky Way stars, although they have a lower metallicity than normal Population I stars in the Milky Way.

text: The stream covers over 100

text: square degree

text: s, and possibly as much as 1,000 square degrees (approximately 5% of the

text: hemisphere

text: visible at any one time, or 5,000 times the area of the

text: full moon

text: ).  Despite its proximity to the

text: solar system

text: and the

text: solid angle

text: that it consequently covers, the stream contains only a few hundred thousand stars.  The low

text: surface brightness

text: of the galaxy (possibly as low as 32.5

text: mag

entity_section: Symbols.2C abbreviations and subdivisions

text: arcmin

text: ²) may have militated against its detection in surveys before SDSS.  The number of stars in the stream is not greatly in excess of a

text: star cluster

text: , and it has been described by a member of the team that discovered it as "a rather pathetic galaxy", in comparison to the Milky Way.  Many of the stars have been known for centuries and thought of as normal Milky Way stars, although they have a lower

text: metallicity

text: than normal

text: Population I

text: stars in the Milky Way.

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answers: NDQ_002605

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answers: NDQ_002610

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answers: NDQ_002620

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answers: NDQ_002624

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answers: NDQ_002625

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answers: NDQ_002626

answers: The low surface brightness of the galaxy

answers: NDQ_002627

answers: It contains only a few hundred thousand stars

answers: NDQ_002628

answers: Star cluster

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: Population I

answers: NDQ_002631

answers: spiral galaxies are generally older than elliptical galaxies

answers: NDQ_002632

answers: The Milky Way

answers: NDQ_002633

answers: The stream contains only a few hundred thousand stars

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answers: The Milky Way

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answers: Milky Way

text: The typical average equipartition strength for spiral galaxies is about 10 μG (microGauss) or 1 nT (nanoTesla). For comparison, the Earth's magnetic field has an average strength of about 0.3 G (Gauss or 30 μT (microTesla)). Radio-faint galaxies like M 31 and M 33, our Milky Way's neighbors, have weaker fields (about 5 μG), while gas-rich galaxies with high star-formation rates, like M 51, M 83 and NGC 6946, have 15 μG on average. In prominent spiral arms the field strength can be up to 25 μG, in regions where also cold gas and dust are concentrated. The strongest total equipartition fields (50-100 μG) were found in starburst galaxies, for example in M 82 and the Antennae, and in nuclear starburst regions, for example in the centers of NGC 1097 and of other barred galaxies.

text: The typical average

text: equipartition strength

text: for

text: spiral galaxies

text: is about 10 μG (

text: microGauss

text: ) or 1 nT (

text: nanoTesla

text: ). For comparison, the Earth's magnetic field has an average strength of about 0.3 G (Gauss or 30 μT (

text: microTesla)

text: ). Radio-faint galaxies like

text: M 31

text: and

text: M 33

text: , our

text: Milky Way

text: 's neighbors, have weaker fields (about 5 μG), while gas-rich galaxies with high star-formation rates, like M 51, M 83 and NGC 6946, have 15 μG on average. In prominent spiral arms the field strength can be up to 25 μG, in regions where also cold gas and dust are concentrated. The strongest total equipartition fields (50-100 μG) were found in

text: starburst galaxies

text: , for example in M 82 and the

text: Antennae

text: , and in nuclear starburst regions, for example in the centers of NGC 1097 and of other

text: barred galaxies

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answers: barred galaxies

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answers: Milky Way

answers: NDQ_002600

answers: gas and dust

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answers: prominent spiral arms

answers: NDQ_002602

answers: starburst

answers: NDQ_002603

answers: elliptical galaxies

answers: NDQ_002604

answers: 10  G

answers: NDQ_002605

answers: cold gas and dust

answers: NDQ_002606

answers: barred

answers: NDQ_002607

answers: galaxies

answers: NDQ_002609

answers: 10  G

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answers: nuclear starburst regions

answers: NDQ_002612

answers: spiral

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answers: galaxies

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answers: Milky Way

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: Milky Way

answers: NDQ_002620

answers: Radio-faint galaxies like M 31 and M 33

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxies

answers: NDQ_002623

answers: Spiral galaxies

answers: NDQ_002624

answers: barred

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: The Earth's magnetic field

answers: NDQ_002627

answers: It's impossible to say

answers: NDQ_002628

answers: Star clusters

answers: NDQ_002629

answers: open star clusters

answers: NDQ_002630

answers: Spiral galaxies

answers: NDQ_002631

answers: Spiral galaxies

answers: NDQ_002632

answers: Our Milky Way's neighbors

answers: NDQ_002633

answers: galaxies with high star-formation rates

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answers: Milky Way

answers: NDQ_002635

answers: The Earth's magnetic field

answers: NDQ_002636

answers: Milky Way

text: After the timeskip, Makken is married to Leite with three children. Sadly, he is killed in the first deep space battle versus the Anti-Spirals, after sacrificing himself to stop a large Anti-Spiral missile from destroying the Super Galaxy Dai-Gurren.

text: After the timeskip, Makken is married to Leite with three children. Sadly, he is killed in the first deep space battle versus the Anti-Spirals, after sacrificing himself to stop a large Anti-Spiral missile from destroying the Super Galaxy Dai-Gurren.

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answers: Galaxy

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answers: three

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answers: spirals

answers: NDQ_002601

answers: spiral

answers: NDQ_002602

answers: Super Galaxy

answers: NDQ_002603

answers: anti-spirals

answers: NDQ_002604

answers: children

answers: NDQ_002605

answers: Galaxy

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answers: Galaxy

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answers: Galaxy

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answers: Galaxy

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answers: Galaxy

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answers: Galaxy Dai-Gurren

answers: NDQ_002624

answers: Dai-Gurren

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: Galaxy

answers: NDQ_002628

answers: Galaxy

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answers: Open star clusters

answers: NDQ_002630

answers: large

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answers: Spiral

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answers: Galaxy Dai-Gurren

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answers: Galaxy

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answers: Spirals

answers: NDQ_002635

answers: Galaxy Dai-Gurren

answers: NDQ_002636

answers: Spirals

text: SAm galaxies are a type of unbarred spiral galaxy, while SBm are a type of barred spiral galaxy. SABm are a type of intermediate spiral galaxy.

text: SAm galaxies are a type of

text: unbarred spiral galaxy

text: , while SBm are a type of

text: barred spiral galaxy

text: . SABm are a type of

text: intermediate spiral galaxy

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answers: 2: The answer has limited relevance and completeness, with significant gaps or inaccuracy.

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answers: barred

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answers: barred spiral galaxy

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answers: barred

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answers: unbarred

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answers: intermediate

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answers: SABm

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answers: billions

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answers: spiral galaxy

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answers: galaxy

answers: NDQ_002617

answers: intermediate spiral galaxy

answers: NDQ_002618

answers: SABm

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answers: intermediate

answers: NDQ_002620

answers: intermediate spiral galaxy

answers: NDQ_002621

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answers: galaxy

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answers: SABm

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answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

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answers: galaxy

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answers: galaxy

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answers: Open star clusters

answers: NDQ_002630

answers: SABm

answers: NDQ_002631

answers: It's impossible to say

answers: NDQ_002632

answers: Smaller galaxies

answers: NDQ_002633

answers: galaxy

answers: NDQ_002634

answers: SABm

answers: NDQ_002635

answers: Our solar system orbits the central disk

answers: NDQ_002636

answers: SABm

text: These are galaxies that look like a stretched-out S shape (or like the integral sign used in calculus). Some objects, such as IC 167, are simply ordinary spiral galaxies viewed from an unusual angle.  Other objects, such as UGC 10770, are interacting pairs of galaxies with tidal tails that look similar to spiral arms.

text: These are galaxies that look like a stretched-out S shape (or like the integral sign used in

text: calculus

text: ). Some objects, such as

text: IC 167

text: , are simply ordinary spiral galaxies viewed from an unusual angle.  Other objects, such as

text: UGC 10770

text: , are interacting pairs of galaxies with tidal tails that look similar to spiral arms.

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answers: 4

answers: NDQ_002598

answers: interacting pairs of galaxies

answers: NDQ_002599

answers: galaxy

answers: NDQ_002600

answers: tidal tails

answers: NDQ_002601

answers: stretched-out S shape

answers: NDQ_002602

answers: ordinary spiral galaxies

answers: NDQ_002603

answers: tidal tails

answers: NDQ_002604

answers: tidal tails

answers: NDQ_002605

answers: spiral

answers: NDQ_002606

answers: stretched-out S shape

answers: NDQ_002607

answers: are galaxies that look like a stretched-out S shape

answers: NDQ_002609

answers: 2 billion galaxies

answers: NDQ_002610

answers: S shape

answers: NDQ_002612

answers: spiral

answers: NDQ_002615

answers: UGC 10770

answers: NDQ_002617

answers: S shape

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: IC 167

answers: NDQ_002620

answers: galaxies

answers: NDQ_002621

answers: galaxies

answers: NDQ_002622

answers: UGC 10770

answers: NDQ_002623

answers: tidal tails

answers: NDQ_002624

answers: integral sign

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Spiral galaxies

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: galaxies

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: UGC 10770

answers: NDQ_002631

answers: It's impossible to say

answers: NDQ_002632

answers: dwarf galaxies

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: Spiral arms

answers: NDQ_002635

answers: Spiral arms

answers: NDQ_002636

answers: stretched-out S shape

text: Pisces Dwarf is an irregular dwarf galaxy that is part of the Local Group.  The galaxy, taking its name from the constellation Pisces where it appears, is suspected of being a satellite galaxy of the Triangulum Galaxy (M33).   It displays a blueshift, as it is approaching the Milky Way at 287 km/s. It may be transition-type galaxy, somewhere between dwarf spheroidal and dwarf irregular. Alternatively, it may be a rare, but statistically acceptable, version of one of the two types.

text: Pisces Dwarf is an

text: irregular

text: dwarf

text: galaxy

text: that is part of the

text: Local Group

text: .  The galaxy, taking its name from the

text: constellation

text: Pisces

text: where it appears, is suspected of being a

text: satellite galaxy

text: of the

text: Triangulum Galaxy

text: (M33).   It displays a

text: blueshift

text: , as it is approaching the

text: Milky Way

text: at 287

text: km/s

text: . It may be transition-type galaxy, somewhere between

text: dwarf spheroidal

text: and

text: dwarf irregular

text: . Alternatively, it may be a rare, but statistically acceptable, version of one of the two types.

answers: tqa2:L_0062/T_0626/0ca13908895d7adcb5d4f7bf27bc2b3a

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answers: irregular dwarf galaxy

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answers: elliptical

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answers: blueshift

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answers: galaxy

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answers: irregular

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answers: Pisces Dwarf

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answers: 287 km/s

answers: NDQ_002610

answers: Triangulum Galaxy

answers: NDQ_002612

answers: Milky Way

answers: NDQ_002615

answers: dwarf galaxy

answers: NDQ_002617

answers: spheroidal

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: Local Group

answers: NDQ_002620

answers: Milky Way

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: dwarf galaxy

answers: NDQ_002623

answers: Pisces Dwarf

answers: NDQ_002624

answers: irregular dwarf galaxy

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The Milky Way

answers: NDQ_002627

answers: It may be transition-type galaxy

answers: NDQ_002628

answers: Local Group

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: dwarf spheroidal

answers: NDQ_002631

answers: irregular

answers: NDQ_002632

answers: satellite galaxy

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answers: Milky Way

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answers: Milky Way

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answers: Milky Way

text: Messier 90 is a member of the Virgo Cluster, being  one of its largest and brightest spiral galaxies, with an absolute magnitude of around -22 (brighter than the Andromeda Galaxy). The galaxy is located approximately 1°.5 away from the subgroup centered on Messier 87.  As a consequence of the galaxy's interaction with the intracluster medium in the Virgo Cluster, the galaxy has lost much of its interstellar medium.  As a result of this process, which is referred to as ram-pressure stripping, the galaxy's interstellar medium and star formation regions appear severely truncated compared to similar galaxies outside the Virgo Cluster and there are even H II regions outside the galactic plane, as well as long (up to 80 kpcs, 260,000 light-years) tails of ionized gas that has been stripped of M90.

text: Messier 90 is a member of the

text: Virgo Cluster

text: , being  one of its largest and brightest spiral galaxies, with an

text: absolute magnitude

text: of around -22 (brighter than the

text: Andromeda Galaxy

text: ). The galaxy is located approximately 1°.5 away from the subgroup centered on

text: Messier 87

text: .  As a consequence of the galaxy's interaction with the

text: intracluster medium

text: in the Virgo Cluster, the galaxy has lost much of its

text: interstellar medium

text: .  As a result of this process, which is referred to as

text: ram-pressure stripping

text: , the galaxy's interstellar medium and

text: star formation region

text: s appear severely truncated compared to similar galaxies outside the Virgo Cluster and there are even

text: H II region

text: s outside the

text: galactic plane

text: , as well as long (up to 80 k

text: pc

text: s, 260,000 light-years) tails of ionized gas that has been stripped of M90.

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answers: 4

answers: NDQ_002598

answers: Virgo Cluster

answers: NDQ_002599

answers: 260,000 light-years

answers: NDQ_002600

answers: star formation regions

answers: NDQ_002601

answers: H II regions outside the galactic plane

answers: NDQ_002602

answers: spiral

answers: NDQ_002603

answers: interstellar medium

answers: NDQ_002604

answers: H II regions outside the galactic plane

answers: NDQ_002605

answers: interstellar

answers: NDQ_002606

answers: intracluster

answers: NDQ_002607

answers: Virgo Cluster

answers: NDQ_002609

answers: 260,000 light-years

answers: NDQ_002610

answers: Virgo Cluster

answers: NDQ_002612

answers: spiral

answers: NDQ_002615

answers: Virgo Cluster

answers: NDQ_002617

answers: Andromeda

answers: NDQ_002618

answers: galaxy's interstellar medium

answers: NDQ_002619

answers: subgroup

answers: NDQ_002620

answers: spiral galaxies

answers: NDQ_002621

answers: Cluster

answers: NDQ_002622

answers: Virgo Cluster

answers: NDQ_002623

answers: Spiral

answers: NDQ_002624

answers: H II

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: The solar system is slowly spinning around our galaxy

answers: NDQ_002627

answers: It is estimated that there are billions of galaxies in the universe

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: largest

answers: NDQ_002631

answers: Spiral galaxies

answers: NDQ_002632

answers: the subgroup centered on Messier 87

answers: NDQ_002633

answers: galaxy's interstellar medium

answers: NDQ_002634

answers: Virgo Cluster

answers: NDQ_002635

answers: galaxy

answers: NDQ_002636

answers: galaxy

text: Passive spiral galaxies (also known as passive spirals) are a type of spiral galaxy located in rich galaxy clusters at high redshifts that present spiral structure, but little or no star formation, in some cases hidden by dust and concentrated within its innermost regions. Often, they seem too to have few or no massive (>20 solar masses) stars.

text: Passive spiral galaxies (also known as passive spirals) are a type of spiral galaxy located in rich galaxy clusters at high

text: redshift

text: s that present spiral structure, but little or no star formation, in some cases hidden by

text: dust

text: and concentrated within its innermost regions. Often, they seem too to have few or no

text: massive

text: solar mass

text: es) stars.

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answers: NDQ_002598

answers: rich galaxy clusters

answers: NDQ_002599

answers: >20 solar masses

answers: NDQ_002600

answers: stars

answers: NDQ_002601

answers: redshifts

answers: NDQ_002602

answers: Passive spiral

answers: NDQ_002603

answers: star formation

answers: NDQ_002604

answers: little or no star formation

answers: NDQ_002605

answers: few or no massive

answers: NDQ_002606

answers: hidden

answers: NDQ_002607

answers: Rich galaxy clusters

answers: NDQ_002609

answers: 20 solar masses

answers: NDQ_002610

answers: galaxy cluster

answers: NDQ_002612

answers: spiral galaxy

answers: NDQ_002615

answers: rich galaxy clusters

answers: NDQ_002617

answers: galaxy clusters

answers: NDQ_002618

answers: galaxy clusters

answers: NDQ_002619

answers: cluster

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answers: high redshifts

answers: NDQ_002621

answers: galaxy clusters

answers: NDQ_002622

answers: galaxy clusters

answers: NDQ_002623

answers: no massive (>20 solar masses) stars

answers: NDQ_002624

answers: galaxy clusters

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: galaxy clusters

answers: NDQ_002628

answers: galaxy clusters

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: solar masses

answers: NDQ_002631

answers: Spiral

answers: NDQ_002632

answers: rich galaxy clusters

answers: NDQ_002633

answers: rich galaxy clusters

answers: NDQ_002634

answers: Spiral galaxy

answers: NDQ_002635

answers: Our solar system orbits the central disk

answers: NDQ_002636

answers: Passive spiral

text: Galaxies in this category are almost always clearly interacting sources. The most famous of these objects is the Whirlpool galaxy (M51; Arp 85), which is composed of a spiral galaxy NGC 5194 that is interacting with a smaller elliptical galaxy NGC 5195. The interaction has distorted the shape of both galaxies; the spiral arm pattern has been enhanced in the larger spiral galaxy, and a bridge of stars and gas has formed between the two galaxies. Many of the other galaxies in this category are also connected by bridges.

text: Galaxies in this category are almost always clearly interacting sources. The most famous of these objects is

text: the Whirlpool galaxy (M51; Arp 85)

text: , which is composed of a spiral galaxy

text: NGC 5194

text: that is interacting with a smaller elliptical galaxy

text: NGC 5195

text: . The interaction has distorted the shape of both galaxies; the spiral arm pattern has been enhanced in the larger spiral galaxy, and a bridge of stars and gas has formed between the two galaxies. Many of the other galaxies in this category are also connected by bridges.

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answers: NDQ_002598

answers: galaxies

answers: NDQ_002599

answers: stars

answers: NDQ_002600

answers: stars and gas

answers: NDQ_002601

answers: bridges

answers: NDQ_002602

answers: spiral galaxy

answers: NDQ_002603

answers: bridge of stars and gas

answers: NDQ_002604

answers: bridges

answers: NDQ_002605

answers: gas

answers: NDQ_002606

answers: distorted

answers: NDQ_002607

answers: Galaxies

answers: NDQ_002609

answers: galaxies

answers: NDQ_002610

answers: interacting sources

answers: NDQ_002612

answers: spiral galaxy

answers: NDQ_002615

answers: Galaxies

answers: NDQ_002617

answers: NGC 5195

answers: NDQ_002618

answers: galaxy

answers: NDQ_002619

answers: elliptical galaxy

answers: NDQ_002620

answers: Galaxy in this category

answers: NDQ_002621

answers: Galaxies

answers: NDQ_002622

answers: Galaxies

answers: NDQ_002623

answers: Galaxies

answers: NDQ_002624

answers: Whirlpool

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The interaction has distorted the shape

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: Galaxies

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: larger spiral galaxy

answers: NDQ_002631

answers: Spiral galaxy

answers: NDQ_002632

answers: Galaxies

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: galaxy

answers: NDQ_002635

answers: galaxy

answers: NDQ_002636

answers: Galaxy in this category

text: A galaxy is a gravitationally bound system of stars, stellar remnants, interstellar gas, dust, and dark matter. The word galaxy is derived from the Greek  (γαλαξίας), literally "milky", a reference to the Milky Way. Galaxies range in size from dwarfs with just a few billion (10) stars to giants with one hundred trillion (10) stars, each orbiting its galaxy's center of mass. Galaxies are categorized according to their visual morphology as elliptical, spiral and irregular. Many galaxies are thought to have black holes at their active centers. The Milky Way's central black hole, known as Sagittarius A*, has a mass four million times greater than the Sun. As of March 2016, GN-z11 is the oldest and most distant observed galaxy with a comoving distance of 32 billion light-years from Earth, and observed as it existed just 400 million years after the Big Bang. Previously, as of July 2015, EGSY8p7 was the most distant known galaxy, estimated to have a light travel distance of 13.2 billion light-years away.

text: A galaxy is a

text: gravitation

text: ally bound system of

text: star

text: s,

text: stellar remnant

text: s,

text: interstellar gas

text: dust

text: , and

text: dark matter

text: . The word galaxy is derived from the

text: Greek

text: (γαλαξίας), literally "milky", a reference to the

text: Milky Way

text: . Galaxies range in size from

text: dwarfs

text: with just a few billion (10) stars to giants with one hundred

text: trillion

text: (10) stars, each orbiting its galaxy's

text: center of mass

text: . Galaxies are categorized according to their visual morphology as

text: elliptical

text: spiral

text: and

text: irregular

text: . Many galaxies are thought to have

text: black hole

text: s at their

text: active centers

text: . The Milky Way's central black hole, known as

text: Sagittarius A*

text: , has a mass four million times greater than the

text: Sun

text: . As of March 2016,

text: is the oldest and most distant observed galaxy with a

text: comoving distance

text: of 32 billion

text: light-years

text: from Earth, and observed as it existed just 400 million years after the Big Bang. Previously, as of July 2015,

text: was the most distant known galaxy, estimated to have a light travel distance of 13.2 billion light-years away.

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answers: Galaxies are categorized according to their visual morphology

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text: The Butcher–Oemler conclusion generated numerous investigations of the cores of rich clusters at intermediate redshift (0.3 ≤ z ≤ 0.9): Couch and Newell (1984), like Butcher and Oemler, acquired broadband photometry of such environments.  Couch et al. (1983), Ellis et al. (1985), MacLaren, Ellis and Couch (1988), Aragon-Salamanca, Ellis and Sharples (1991) and Aragon-Salamanca et al. (1993) imaged clusters with redshifts between 0.5 ≤ z ≤ 0.9 in both optical and infrared bands.  Spectroscopic observations were conducted by Dressler and Gunn (1982), Lavery and Henry (1985) and Couch and Sharples (1987).  Studies of the morphologies of the galaxies in the cores of these clusters were undertaken using the Hubble Space Telescope by Couch et al. (1994) and Dressler et al. (1994).  The outcome of these investigations is that the Butcher–Oemler effect is widespread in rich clusters at z > 0.2 and is due to vigorous episodes of star formation in a subset of the cluster members.

text: The Butcher–Oemler conclusion generated numerous investigations of the cores of rich clusters at intermediate redshift (0.3 ≤ z ≤ 0.9):

text: Couch

text: and Newell (1984), like Butcher and Oemler, acquired broadband photometry of such environments.  Couch et al. (1983), Ellis et al. (1985), MacLaren,

text: Ellis

text: and Couch (1988), Aragon-Salamanca, Ellis and Sharples (1991) and Aragon-Salamanca et al. (1993) imaged clusters with redshifts between 0.5 ≤ z ≤ 0.9 in both

text: optical

text: and

text: infrared

text: bands.

text: Spectroscopic

text: observations were conducted by Dressler and

text: Gunn

text: (1982), Lavery and Henry (1985) and Couch and Sharples (1987).  Studies of the

text: morphologies

text: of the galaxies in the cores of these clusters were undertaken using the

text: Hubble Space Telescope

text: by Couch et al. (1994) and Dressler et al. (1994).  The outcome of these investigations is that the Butcher–Oemler effect is widespread in rich clusters at z > 0.2 and is due to vigorous episodes of star formation in a subset of the cluster members.

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answers: rich clusters

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answers: rich clusters

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answers: vigorous episodes of star formation

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answers: rich clusters at intermediate redshift

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answers: 900 billion galaxies

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answers: NDQ_002617

answers: rich clusters

answers: NDQ_002618

answers: Hubble Space Telescope

answers: NDQ_002619

answers: cluster

answers: NDQ_002620

answers: Butcher–Oemler effect

answers: NDQ_002621

answers: clusters

answers: NDQ_002622

answers: rich clusters

answers: NDQ_002623

answers: Butcher–Oemler effect

answers: NDQ_002624

answers: intermediate redshift

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: The Butcher–Oemler conclusion

answers: NDQ_002627

answers: The Butcher–Oemler effect is widespread in rich clusters

answers: NDQ_002628

answers: galaxies

answers: NDQ_002629

answers: open star clusters

answers: NDQ_002630

answers: clusters

answers: NDQ_002631

answers: The Butcher–Oemler conclusion

answers: NDQ_002632

answers: The Butcher–Oemler effect is widespread in rich clusters

answers: NDQ_002633

answers: Rich clusters at intermediate redshift

answers: NDQ_002634

answers: The Butcher–Oemler effect

answers: NDQ_002635

answers: The Hubble Space Telescope

answers: NDQ_002636

answers: z > 0.2

text: Observational evidence for this galaxy was presented in 2015, based on the claimed discovery of four, Cepheid variable stars by Sukanya Chakrabarti (RIT) and collaborators. Search for the stars was motivated by an earlier study  that linked a warp in the HI (atomic hydrogen) disk of the Milky Way Galaxy to the tidal effects of a perturbing galaxy. The unseen perturber's mass was calculated to be about 1% of that of the Milky Way, which would make it the third heaviest satellite of the Milky Way, after the Magellanic Clouds (LMC and SMC, each some 10x larger than Galaxy X). In this theoretical model, the putative satellite galaxy would have interacted with the Milky Way some 600 million years ago, coming as close as , and would now be on its way away from the Milky Way.

text: Observational evidence for this galaxy was presented in 2015, based on the claimed discovery of four, Cepheid variable stars by Sukanya Chakrabarti

text: (RIT)

text: and collaborators. Search for the stars was motivated by an earlier study  that linked a warp in the HI (atomic hydrogen) disk of the Milky Way Galaxy to the tidal effects of a perturbing galaxy. The unseen perturber's mass was calculated to be about 1% of that of the Milky Way, which would make it the third heaviest satellite of the Milky Way, after the

text: Magellanic Clouds

text: (LMC and SMC, each some 10x larger than Galaxy X). In this theoretical model, the putative satellite galaxy would have interacted with the Milky Way some 600 million years ago, coming as close as , and would now be on its way away from the Milky Way.

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answers: Cepheid

answers: NDQ_002599

answers: four

answers: NDQ_002600

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answers: NDQ_002601

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answers: NDQ_002602

answers: Milky Way Galaxy

answers: NDQ_002603

answers: gas and dust

answers: NDQ_002604

answers: a warp

answers: NDQ_002605

answers: variable stars

answers: NDQ_002606

answers: galaxy

answers: NDQ_002607

answers: Galaxy X

answers: NDQ_002609

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answers: NDQ_002610

answers: Galaxy X

answers: NDQ_002612

answers: Milky Way Galaxy

answers: NDQ_002615

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answers: NDQ_002617

answers: Galaxy X

answers: NDQ_002618

answers: Galaxy

answers: NDQ_002619

answers: satellite

answers: NDQ_002620

answers: Milky Way Galaxy

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: Galaxy X

answers: NDQ_002623

answers: Galaxy X

answers: NDQ_002624

answers: Cepheid

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The unseen perturber's mass

answers: NDQ_002627

answers: Galaxy X

answers: NDQ_002628

answers: Galaxy

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: Magellanic Clouds

answers: NDQ_002631

answers: Galaxy X

answers: NDQ_002632

answers: Galaxy X

answers: NDQ_002633

answers: Galaxy X

answers: NDQ_002634

answers: Milky Way Galaxy

answers: NDQ_002635

answers: The Milky Way Galaxy

answers: NDQ_002636

answers: Milky Way Galaxy

text: Andromeda Galaxy appears to have significantly more common stars than the Milky Way, seeming to predominate the old stars with ages >7 years. The estimated luminosity of Andromeda Galaxy, , is about 25% higher than that of our own galaxy. However, the galaxy has a high inclination as seen from Earth and its interstellar dust absorbs an unknown amount of light, so it is difficult to estimate its actual brightness and other authors have given other values for the luminosity of the Andromeda Galaxy (including to propose it is the second brightest galaxy within a radius of 10 mega parsecs of the Milky Way, after the Sombrero Galaxy, with an absolute magnitude of around -22.21 or close)

text: Andromeda Galaxy appears to have significantly more common stars than the Milky Way, seeming to predominate the old stars with ages >7 years. The estimated

text: luminosity

text: of Andromeda Galaxy, , is about 25% higher than that of our own galaxy. However, the galaxy has a high

text: inclination

text: as seen from Earth and its

text: interstellar dust

text: absorbs an unknown amount of light, so it is difficult to estimate its actual brightness and other authors have given other values for the luminosity of the Andromeda Galaxy (including to propose it is the second brightest galaxy within a radius of 10

text: mega

text: parsec

text: s of the Milky Way, after the

text: Sombrero Galaxy

text: , with an absolute magnitude of around -22.21 or close)

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answers: stars

answers: NDQ_002601

answers: high inclination

answers: NDQ_002602

answers: Milky Way

answers: NDQ_002603

answers: the Milky Way

answers: NDQ_002604

answers: high inclination

answers: NDQ_002605

answers: old stars

answers: NDQ_002606

answers: Galaxy

answers: NDQ_002607

answers: Milky Way

answers: NDQ_002609

answers: stars

answers: NDQ_002610

answers: Andromeda Galaxy

answers: NDQ_002612

answers: Milky Way

answers: NDQ_002615

answers: Galaxy

answers: NDQ_002617

answers: Milky Way

answers: NDQ_002618

answers: The estimated luminosity of Andromeda Galaxy

answers: NDQ_002619

answers: galaxy

answers: NDQ_002620

answers: Milky Way

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: Galaxy

answers: NDQ_002623

answers: Milky Way

answers: NDQ_002624

answers: Andromeda

answers: NDQ_002625

answers: Andromeda Galaxy

answers: NDQ_002626

answers: The galaxy has a high inclination as seen from Earth

answers: NDQ_002627

answers: It is difficult to estimate its actual brightness

answers: NDQ_002628

answers: Galaxy

answers: NDQ_002629

answers: Open star clusters contain more stars

answers: NDQ_002630

answers: galaxy

answers: NDQ_002631

answers: Andromeda Galaxy

answers: NDQ_002632

answers: Andromeda Galaxy

answers: NDQ_002633

answers: It is difficult to estimate its actual brightness

answers: NDQ_002634

answers: Milky Way

answers: NDQ_002635

answers: The Milky Way

answers: NDQ_002636

answers: Milky Way

text: In all methods the size is an indirect measure, obtained by a model that transforms, in abstract way, the real particle shape into a simple and standarized shape, like a sphere (the most usual) or a cuboid (when minimum bounding box is used), where the size parameter (ex. diameter of sphere) makes sense.  Exception is the mathematical morphology approach, where no shape hypothesis is necessary.

text: In all methods the size is an indirect measure, obtained by a model that transforms, in abstract way, the real particle shape into a simple and standarized shape, like a sphere (the most usual) or a

text: cuboid

text: (when

text: minimum bounding box

text: is used), where the size parameter (ex. diameter of sphere) makes sense.  Exception is the

text: mathematical morphology approach

text: , where no shape hypothesis is necessary.

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answers: 0

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answers: 0

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answers: 0

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answers: 0

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answers: 0

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answers: 0

answers: tqa2:L_0062/T_0631/2a2ce10e5e1955e321e5e9a61965aa68

answers: 0

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answers: 0

answers: tqa2:L_0062/T_0631/5939595f5f3ebee0b7bd227abde4cf5f

answers: 0

answers: tqa2:L_0062/T_0632/c8a77a90f4220bb2ba198c9463f6e78d

answers: 0

answers: tqa2:L_0062/T_0632/468f2f1df85c20ecbef75cba93c0f9e0

answers: 0

answers: tqa2:L_0062/T_0632/27861f32ee4587789c46601b43d220bd

answers: 0

answers: tqa2:L_0062/T_0632/e5a5617ff15554e1863e0947fc9df3d0

answers: 0

answers: tqa2:L_0062/T_0632/76a4d20633cfa7e3d87362f8d2ec771b

answers: 0

answers: tqa2:L_0062/T_0632/312dd58a52ea7bdc18423e16b71e736d

answers: 0

answers: tqa2:L_0062/T_0632/07df44424134e44a91809881a664b81a

answers: 0

answers: tqa2:L_0062/T_0632/24cc00a29e23692d56b0664eeefac3e9

answers: 0

answers: tqa2:L_0062/T_0632/4d920cc8ec5fa1ec4415ceeec8a09cd4

answers: 0

answers: tqa2:L_0062/T_0632/ebe6be9a54bc05aec692ea3fb22fbfd0

answers: 0

answers: NDQ_002598

answers: 0

answers: NDQ_002599

answers: 0

answers: NDQ_002600

answers: 0

answers: NDQ_002601

answers: 0

answers: NDQ_002602

answers: 0

answers: NDQ_002603

answers: 0

answers: NDQ_002604

answers: 0

answers: NDQ_002605

answers: 0

answers: NDQ_002606

answers: 0

answers: NDQ_002607

answers: 0

answers: NDQ_002609

answers: 0

answers: NDQ_002610

answers: 0

answers: NDQ_002612

answers: 0

answers: NDQ_002615

answers: 0

answers: NDQ_002617

answers: 0

answers: NDQ_002618

answers: 0

answers: NDQ_002619

answers: 0

answers: NDQ_002620

answers: 3

answers: NDQ_002621

answers: 0

answers: NDQ_002622

answers: 0

answers: NDQ_002623

answers: 0

answers: NDQ_002624

answers: 0

answers: NDQ_002625

answers: 0

answers: NDQ_002626

answers: 0

answers: NDQ_002627

answers: 0

answers: NDQ_002628

answers: 4

answers: NDQ_002629

answers: 3

answers: NDQ_002630

answers: 0

answers: NDQ_002631

answers: 2

answers: NDQ_002632

answers: 2

answers: NDQ_002633

answers: 0

answers: NDQ_002634

answers: 0

answers: NDQ_002635

answers: 0

answers: NDQ_002636

answers: 0

answers: NDQ_002598

answers: cuboid

answers: NDQ_002599

answers: billions

answers: NDQ_002600

answers: no shape hypothesis

answers: NDQ_002601

answers: mathematical morphology

answers: NDQ_002602

answers: sphere

answers: NDQ_002603

answers: no shape hypothesis is necessary

answers: NDQ_002604

answers: no shape hypothesis

answers: NDQ_002605

answers: particles

answers: NDQ_002606

answers: Exception

answers: NDQ_002607

answers: a sphere

answers: NDQ_002609

answers: billions of stars

answers: NDQ_002610

answers: sphere

answers: NDQ_002612

answers: sphere

answers: NDQ_002615

answers: Cuboid

answers: NDQ_002617

answers: cuboid

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: a sphere

answers: NDQ_002620

answers: a sphere

answers: NDQ_002621

answers: cuboid

answers: NDQ_002622

answers: Cuboid

answers: NDQ_002623

answers: no shape hypothesis is necessary

answers: NDQ_002624

answers: mathematical morphology

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: The size is an indirect measure

answers: NDQ_002627

answers: The size is an indirect measure

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: globular star clusters

answers: NDQ_002630

answers: diameter of sphere

answers: NDQ_002631

answers: no shape hypothesis is necessary

answers: NDQ_002632

answers: dwarf galaxies

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: galaxy

answers: NDQ_002635

answers: orbits the central disk

answers: NDQ_002636

answers: no shape hypothesis is necessary

text: Although the description of the objects in this category implies that the galaxies are separating apart, most of these galaxies are merging. Many of the objects have very pronounced tidal tails and bridges that have formed as a consequence of the interaction. Most objects are in the early stages of the merging process, where the galaxies still appear to have distinct nuclei and distinct (albeit distorted) disks. Among the most notable galaxies in this category are the Antennae Galaxies (NGC 4038 and NGC 4039, Arp 244) and the Mice Galaxies (NGC 4676, Arp 242).

text: Although the description of the objects in this category implies that the galaxies are separating apart, most of these galaxies are merging. Many of the objects have very pronounced tidal tails and bridges that have formed as a consequence of the interaction. Most objects are in the early stages of the merging process, where the galaxies still appear to have distinct nuclei and distinct (albeit distorted) disks. Among the most notable galaxies in this category are the

text: Antennae Galaxies

text: (NGC 4038 and NGC 4039, Arp 244) and the

text: Mice Galaxies

text: (NGC 4676, Arp 242).

answers: tqa2:L_0062/T_0626/0ca13908895d7adcb5d4f7bf27bc2b3a

answers: 0

answers: tqa2:L_0062/T_0626/aa230dccf7df24426100f44ce03103ce

answers: 0

answers: tqa2:L_0062/T_0626/0bc87a3d9bd80939942d41fd2b980314

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answers: tqa2:L_0062/T_0626/a3a9a07ef08d0f22e18ef84af974cf2b

answers: 0

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answers: 0

answers: tqa2:L_0062/T_0626/2f858cab18ffdd6b016f596331483e6d

answers: 0

answers: tqa2:L_0062/T_0626/6701fd507aeea0d27536bfec8819d5ba

answers: 0

answers: tqa2:L_0062/T_0626/f44525a6616d61dee8726714e6b3ab8a

answers: 0

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answers: 0

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answers: 0

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answers: 4

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answers: 0

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answers: 0

answers: tqa2:L_0062/T_0632/76a4d20633cfa7e3d87362f8d2ec771b

answers: 4

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answers: 0

answers: tqa2:L_0062/T_0632/07df44424134e44a91809881a664b81a

answers: 0

answers: tqa2:L_0062/T_0632/24cc00a29e23692d56b0664eeefac3e9

answers: 4

answers: tqa2:L_0062/T_0632/4d920cc8ec5fa1ec4415ceeec8a09cd4

answers: 0

answers: tqa2:L_0062/T_0632/ebe6be9a54bc05aec692ea3fb22fbfd0

answers: 0

answers: NDQ_002598

answers: 0

answers: NDQ_002599

answers: 0

answers: NDQ_002600

answers: 4

answers: NDQ_002601

answers: 0

answers: NDQ_002602

answers: 4

answers: NDQ_002603

answers: 0

answers: NDQ_002604

answers: 4

answers: NDQ_002605

answers: 0

answers: NDQ_002606

answers: 0

answers: NDQ_002607

answers: 4

answers: NDQ_002609

answers: 0

answers: NDQ_002610

answers: 0

answers: NDQ_002612

answers: 0

answers: NDQ_002615

answers: 1

answers: NDQ_002617

answers: 0

answers: NDQ_002618

answers: 0

answers: NDQ_002619

answers: 0

answers: NDQ_002620

answers: 4

answers: NDQ_002621

answers: 0

answers: NDQ_002622

answers: 0

answers: NDQ_002623

answers: 0

answers: NDQ_002624

answers: 0

answers: NDQ_002625

answers: 0

answers: NDQ_002626

answers: 0

answers: NDQ_002627

answers: 4

answers: NDQ_002628

answers: 4

answers: NDQ_002629

answers: 4

answers: NDQ_002630

answers: 4

answers: NDQ_002631

answers: 3

answers: NDQ_002632

answers: 3

answers: NDQ_002633

answers: 4

answers: NDQ_002634

answers: 0

answers: NDQ_002635

answers: 0

answers: NDQ_002636

answers: 4

answers: NDQ_002598

answers: galaxies

answers: NDQ_002599

answers: galaxy

answers: NDQ_002600

answers: tidal tails and bridges

answers: NDQ_002601

answers: distorted) disks

answers: NDQ_002602

answers: Antennae Galaxies

answers: NDQ_002603

answers: the galaxies are separating apart

answers: NDQ_002604

answers: tidal tails and bridges

answers: NDQ_002605

answers: nuclei

answers: NDQ_002606

answers: distorted

answers: NDQ_002607

answers: galaxies

answers: NDQ_002609

answers: galaxies

answers: NDQ_002610

answers: galaxies are merging

answers: NDQ_002612

answers: Galaxies

answers: NDQ_002615

answers: galaxies

answers: NDQ_002617

answers: Antennae

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: galaxies

answers: NDQ_002620

answers: galaxies are separating apart

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxies

answers: NDQ_002623

answers: galaxies are separating apart

answers: NDQ_002624

answers: Antennae

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Tidal

answers: NDQ_002627

answers: galaxies

answers: NDQ_002628

answers: Galaxies

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: Galaxies

answers: NDQ_002631

answers: Spiral galaxies

answers: NDQ_002632

answers: galaxies are separating apart

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: galaxy

answers: NDQ_002635

answers: galaxies are separating apart

answers: NDQ_002636

answers: NGC 4038 and NGC 4039

text: The northern main spiral arm contains four large HII regions, while the southern arm has greater concentrations of young, hot stars. The estimated rate of supernova explosions in the Triangulum Galaxy is 0.06 Type Ia and 0.62 Type Ib/Type II per century. This is equivalent to a supernova explosion every 147 years, on average. As of 2008, a total of 100 supernova remnants have been identified in the Triangulum Galaxy, the majority of which lies in the southern half of the spiral galaxy. Similar asymmetries exist for H I and H II regions, plus highly luminous concentrations of massive, O type stars. The center of the distribution of these features is offset about two arc minutes to the southwest. M33 being a local galaxy, the Central Bureau for Astronomical Telegrams (CBAT) tracks novae in it along with M31 and M81.

text: The northern main spiral arm contains four large

text: HII region

text: s, while the southern arm has greater concentrations of young, hot stars. The estimated rate of

text: supernova

text: explosions in the Triangulum Galaxy is 0.06

text: Type Ia

text: and 0.62

text: Type Ib

text: Type II

text: per century. This is equivalent to a supernova explosion every 147 years, on average. As of 2008, a total of 100

text: supernova remnant

text: s have been identified in the Triangulum Galaxy, the majority of which lies in the southern half of the spiral galaxy. Similar asymmetries exist for H I and H II regions, plus highly luminous concentrations of massive,

text: O type stars

text: . The center of the distribution of these features is offset about two arc minutes to the southwest. M33 being a local galaxy, the

entity_name: Central Bureau for Astronomical Telegrams

text: Central Bureau for Astronomical Telegrams

text: (CBAT) tracks

text: nova

text: e in it along with M31 and

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answers: 4

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answers: NDQ_002636

answers: 4

answers: NDQ_002598

answers: HII regions

answers: NDQ_002599

answers: galaxy

answers: NDQ_002600

answers: novae

answers: NDQ_002601

answers: offset about two arc minutes to the southwest

answers: NDQ_002602

answers: spiral galaxy

answers: NDQ_002603

answers: young, hot stars

answers: NDQ_002604

answers: large HII regions

answers: NDQ_002605

answers: young, hot

answers: NDQ_002606

answers: galaxy

answers: NDQ_002607

answers: HII regions

answers: NDQ_002609

answers: 100 billion stars

answers: NDQ_002610

answers: supernova

answers: NDQ_002612

answers: spiral galaxy

answers: NDQ_002615

answers: large HII regions

answers: NDQ_002617

answers: Triangulum

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: local galaxy

answers: NDQ_002620

answers: Triangulum Galaxy

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: large HII regions

answers: NDQ_002623

answers: elliptical

answers: NDQ_002624

answers: local galaxy

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: This is equivalent to a supernova explosion every 147 years, on average

answers: NDQ_002627

answers: It is estimated that there are billions of galaxies

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: open star clusters

answers: NDQ_002630

answers: large

answers: NDQ_002631

answers: Spiral galaxies

answers: NDQ_002632

answers: M33 being a local galaxy

answers: NDQ_002633

answers: It is equivalent to a supernova explosion every 147 years

answers: NDQ_002634

answers: The southern arm

answers: NDQ_002635

answers: The Triangulum Galaxy

answers: NDQ_002636

answers: Triangulum Galaxy

text: An estimation of the galaxy's span resulted in a conclusion of 150,000 light years, which is slightly larger than the Milky Way.

text: An estimation of the galaxy's span resulted in a conclusion of 150,000

text: light year

text: s, which is slightly larger than the Milky Way.

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answers: 2: The answer has limited relevance and completeness, with significant gaps or inaccuracy.

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answers: galaxy

answers: NDQ_002599

answers: 150,000

answers: NDQ_002600

answers: Milky Way

answers: NDQ_002601

answers: slightly larger than the Milky Way

answers: NDQ_002602

answers: Milky Way

answers: NDQ_002603

answers: galaxy's span

answers: NDQ_002604

answers: 150,000 light years

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answers: galaxy

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answers: galaxy

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answers: galaxy

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answers: 150,000 light years

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answers: The Milky Way

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answers: The Milky Way

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answers: galaxy's span

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answers: Open star clusters

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answers: Milky Way

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answers: The Milky Way

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answers: Milky Way

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answers: galaxy's span

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answers: The Milky Way

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answers: Milky Way

text: The size and shape of a cooking vessel is typically determined by how it will be used. Cooking vessels are typically referred to as "pots" and "pans," but there is great variation in their actual shapes. Most cooking vessels are roughly cylindrical.

text: The size and shape of a cooking vessel is typically determined by how it will be used. Cooking vessels are typically referred to as "pots" and "pans," but there is great variation in their actual shapes. Most cooking vessels are roughly

text: cylindrical

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answers: It is not possible to tell.

answers: NDQ_002624

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answers: Most cooking vessels are roughly cylindrical

answers: NDQ_002626

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answers: There is great variation in their actual shapes. Most cooking vessels are roughly cylindrical

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answers: Our solar system orbits the central disk of our galaxy

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text: The 25 target galaxies are chosen to be representative (i.e. cover the range of basic galaxy parameters and environments) of nearby (distance < 27 Mpc) early type (E and S0) galaxies. The survey also includes 3 `bonus’ galaxies which have been observed during times that the main sample galaxies are not available. All galaxies are accessible from the northern hemisphere. Although only a small sample, the data reach to large galactocentric radii with excellent velocity resolution and S/N compared to other surveys.

text: The 25 target galaxies are chosen to be representative (i.e. cover the range of basic galaxy parameters and environments) of nearby (distance < 27 Mpc) early type (E and S0) galaxies. The survey also includes 3 `bonus’ galaxies which have been observed during times that the main sample galaxies are not available. All galaxies are accessible from the northern hemisphere. Although only a small sample, the data reach to large galactocentric radii with excellent velocity resolution and

text: S/N

text: compared to other surveys.

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text: The morphological type of NGC 5238 has been the subject of some controversy. In 1979, the galaxy was classified as a barred spiral galaxy. Soon after, in 1984, the galaxy was included in a study of blue compact dwarf galaxies, incompatible with the classification of a barred spiral. However, the barred spiral classification was considered the correct classification for years. It was not until the mid 1990s that the galaxy was first recognized as a dwarf irregular galaxy. Even after this, the majority of studies recognized the galaxy as a spiral galaxy until 2015, when the classification of irregular finally became widely accepted

text: The morphological type of NGC 5238 has been the subject of some controversy. In 1979, the galaxy was classified as a

text: barred spiral

text: galaxy. Soon after, in 1984, the galaxy was included in a study of

text: blue compact dwarf

text: galaxies, incompatible with the classification of a barred spiral. However, the barred spiral classification was considered the correct classification for years. It was not until the mid 1990s that the galaxy was first recognized as a

text: dwarf irregular galaxy

text: . Even after this, the majority of studies recognized the galaxy as a spiral galaxy until 2015, when the classification of irregular finally became widely accepted

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text: A Supercluster is a  large group of smaller galaxy clusters or galaxy groups, which is among the largest-known structures of the cosmos. The Milky Way is part of the Local Group galaxy cluster (that contains more than 54 galaxies), which in turn is part of the Laniakea Supercluster. This supercluster spans over 500 million light-years, while the Local Group spans over 10 million light-years. The number of superclusters in the observable universe is estimated to be 10 million.

text: A Supercluster is a  large group of smaller

text: galaxy cluster

text: s or

text: galaxy group

text: s, which is among the

text: largest-known structures

text: of the

text: cosmos

text: . The

text: Milky Way

text: is part of the

text: Local Group

text: galaxy cluster

text: (that contains more than 54 galaxies), which in turn is part of the

text: Laniakea Supercluster

text: . This supercluster spans over 500 million

text: light-year

text: s, while the Local Group spans over 10 million light-years. The number of superclusters in the observable universe is estimated to be 10 million.

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answers: NDQ_002622

answers: galaxy cluster

answers: NDQ_002623

answers: The Milky Way

answers: NDQ_002624

answers: The Milky Way

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: The Milky Way

answers: NDQ_002627

answers: It is estimated to be 10 million

answers: NDQ_002628

answers: galaxy clusters

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: Supercluster

answers: NDQ_002631

answers: The Milky Way

answers: NDQ_002632

answers: The Milky Way

answers: NDQ_002633

answers: Galaxy clusters or galaxy groups

answers: NDQ_002634

answers: The Milky Way

answers: NDQ_002635

answers: The Milky Way

answers: NDQ_002636

answers: The Milky Way

text: Approximately 77% of observed galaxies are spiral galaxies, two-thirds of all spiral galaxies are barred, and more than half, like the Milky Way, exhibit multiple arms. What makes our galaxy different, according to Rare Earth, is that it is unusually quiet and dim (see argument below), representing just 7% of its kind. Even so, this would still represent more than 200 billion galaxies in the known universe.

text: Approximately 77% of observed galaxies are spiral galaxies, two-thirds of all spiral galaxies are barred, and more than half, like the Milky Way, exhibit multiple arms. What makes our galaxy different, according to Rare Earth, is that it is unusually quiet and dim (see argument below), representing just 7% of its kind. Even so, this would still represent more than 200 billion galaxies in the known universe.

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answers: NDQ_002598

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answers: NDQ_002599

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answers: NDQ_002600

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answers: NDQ_002601

answers: 0

answers: NDQ_002602

answers: 4

answers: NDQ_002603

answers: 0

answers: NDQ_002604

answers: 4

answers: NDQ_002605

answers: 0

answers: NDQ_002606

answers: 4

answers: NDQ_002607

answers: 0

answers: NDQ_002609

answers: 4

answers: NDQ_002610

answers: 4

answers: NDQ_002612

answers: 4

answers: NDQ_002615

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answers: NDQ_002617

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answers: NDQ_002618

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answers: NDQ_002619

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answers: NDQ_002620

answers: 2

answers: NDQ_002621

answers: 4

answers: NDQ_002622

answers: 0

answers: NDQ_002623

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answers: NDQ_002624

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answers: NDQ_002625

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answers: NDQ_002626

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answers: NDQ_002627

answers: 5

answers: NDQ_002628

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answers: 3

answers: NDQ_002631

answers: 4

answers: NDQ_002632

answers: 2

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answers: 4

answers: NDQ_002634

answers: 4

answers: NDQ_002635

answers: 0

answers: NDQ_002636

answers: 4

answers: NDQ_002598

answers: barred

answers: NDQ_002599

answers: 200 billion

answers: NDQ_002600

answers: barred

answers: NDQ_002601

answers: multiple arms

answers: NDQ_002602

answers: Spiral galaxies

answers: NDQ_002603

answers: the Milky Way

answers: NDQ_002604

answers: multiple arms

answers: NDQ_002605

answers: barred

answers: NDQ_002606

answers: galaxies

answers: NDQ_002607

answers: are spiral galaxies

answers: NDQ_002609

answers: 200 billion galaxies

answers: NDQ_002610

answers: Milky Way

answers: NDQ_002612

answers: spiral

answers: NDQ_002615

answers: Milky Way

answers: NDQ_002617

answers: Milky Way

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: galaxy

answers: NDQ_002620

answers: Spiral galaxies

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: Milky Way

answers: NDQ_002623

answers: The Milky Way

answers: NDQ_002624

answers: Milky Way

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The Milky Way

answers: NDQ_002627

answers: 200 billion galaxies

answers: NDQ_002628

answers: star clusters

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: Spiral galaxies

answers: NDQ_002631

answers: Spiral galaxies

answers: NDQ_002632

answers: Milky Way

answers: NDQ_002633

answers: 200 billion

answers: NDQ_002634

answers: The Milky Way

answers: NDQ_002635

answers: The Milky Way

answers: NDQ_002636

answers: The Milky Way

text: The first intergalactic stars were discovered in the Virgo cluster of galaxies. These stars form a massive group approximately 300,000 light years away from the nearest galaxy.

text: The first intergalactic stars were discovered in the Virgo cluster of galaxies. These stars form a massive group approximately 300,000

text: light year

text: s away from the nearest galaxy.

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answers: 3: The answer has limited relevance and completeness, with noticeable gaps or inaccuracy.

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answers: 4

answers: NDQ_002598

answers: galaxies

answers: NDQ_002599

answers: 300,000

answers: NDQ_002600

answers: stars

answers: NDQ_002601

answers: massive group

answers: NDQ_002602

answers: Virgo cluster

answers: NDQ_002603

answers: elliptical

answers: NDQ_002604

answers: stars

answers: NDQ_002605

answers: massive group

answers: NDQ_002606

answers: cluster

answers: NDQ_002607

answers: galaxies

answers: NDQ_002609

answers: 3 billion stars

answers: NDQ_002610

answers: Virgo cluster

answers: NDQ_002612

answers: galaxy

answers: NDQ_002615

answers: Virgo cluster

answers: NDQ_002617

answers: Virgo

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: intergalactic

answers: NDQ_002620

answers: massive group

answers: NDQ_002621

answers: galaxies

answers: NDQ_002622

answers: Virgo cluster

answers: NDQ_002623

answers: Virgo

answers: NDQ_002624

answers: intergalactic

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: galaxies

answers: NDQ_002628

answers: galaxies

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: massive

answers: NDQ_002631

answers: Virgo

answers: NDQ_002632

answers: Dwarf galaxies

answers: NDQ_002633

answers: Virgo cluster

answers: NDQ_002634

answers: Virgo

answers: NDQ_002635

answers: Our solar system orbits the central disk

answers: NDQ_002636

answers: galaxy

text: The galaxy is inclined an estimated 77° relative to the Earth (where an angle of 90° would be viewed directly from the side). Analysis of the cross-sectional shape of the galaxy appears to demonstrate a pronounced, S-shaped warp, rather than just a flat disk. A possible cause of such a warp could be gravitational interaction with the satellite galaxies near the Andromeda Galaxy. The galaxy M33 could be responsible for some warp in Andromeda's arms, though more precise distances and radial velocities are required.

text: The galaxy is inclined an estimated 77° relative to the Earth (where an angle of 90° would be viewed directly from the side). Analysis of the cross-sectional shape of the galaxy appears to demonstrate a pronounced, S-shaped warp, rather than just a flat disk. A possible cause of such a warp could be gravitational interaction with the satellite galaxies near the Andromeda Galaxy. The galaxy

text: could be responsible for some warp in Andromeda's arms, though more precise distances and radial velocities are required.

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answers: NDQ_002598

answers: galaxy M33

answers: NDQ_002599

answers: galaxy

answers: NDQ_002600

answers: galaxy

answers: NDQ_002601

answers: S-shaped warp

answers: NDQ_002602

answers: galaxy M33

answers: NDQ_002603

answers: gravitational interaction

answers: NDQ_002604

answers: pronounced, S-shaped warp

answers: NDQ_002605

answers: galaxy

answers: NDQ_002606

answers: galaxy

answers: NDQ_002607

answers: Galaxy M33

answers: NDQ_002609

answers: billions of stars

answers: NDQ_002610

answers: galaxy M33

answers: NDQ_002612

answers: galaxy

answers: NDQ_002615

answers: galaxy

answers: NDQ_002617

answers: galaxy M33

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: galaxies

answers: NDQ_002620

answers: Galaxy M33

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxy

answers: NDQ_002623

answers: galaxy M33 could be responsible for some warp

answers: NDQ_002624

answers: galaxy M33

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: An estimated 77° relative to the Earth

answers: NDQ_002627

answers: galaxy M33 could be responsible for some warp

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: galaxy M33

answers: NDQ_002631

answers: S-shaped warp

answers: NDQ_002632

answers: Andromeda Galaxy

answers: NDQ_002633

answers: galaxy

answers: NDQ_002634

answers: galaxy M33

answers: NDQ_002635

answers: The galaxy

answers: NDQ_002636

answers: a pronounced, S-shaped warp

text: Patterns, sometimes called developments, show the size and shape of a flat piece of material needed for later bending or folding into a three dimensional shape.

text: Patterns, sometimes called developments, show the size and shape of a flat piece of material needed for later bending or folding into a three dimensional shape.

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answers: NDQ_002598

answers: Patterns

answers: NDQ_002599

answers: three dimensional

answers: NDQ_002600

answers: patterns

answers: NDQ_002601

answers: later bending

answers: NDQ_002602

answers: three dimensional

answers: NDQ_002603

answers: flat piece of material

answers: NDQ_002604

answers: three dimensional shape

answers: NDQ_002605

answers: flat

answers: NDQ_002606

answers: Patterns

answers: NDQ_002607

answers: are a type of galaxy

answers: NDQ_002609

answers: billions of stars

answers: NDQ_002610

answers: galaxy

answers: NDQ_002612

answers: three dimensional

answers: NDQ_002615

answers: Patterns

answers: NDQ_002617

answers: Patterns

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: Patterns

answers: NDQ_002620

answers: dwarf galaxies

answers: NDQ_002621

answers: Patterns

answers: NDQ_002622

answers: Patterns

answers: NDQ_002623

answers: elliptical

answers: NDQ_002624

answers: Patterns

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is rotating around our galaxy.

answers: NDQ_002627

answers: galaxies

answers: NDQ_002628

answers: Star clusters

answers: NDQ_002629

answers: globular

answers: NDQ_002630

answers: unanswerable

answers: NDQ_002631

answers: elliptical

answers: NDQ_002632

answers: Dwarf galaxies

answers: NDQ_002633

answers: galaxy

answers: NDQ_002634

answers: The solar system is in the Milky Way galaxy.

answers: NDQ_002635

answers: Our solar system orbits the central disk of our galaxy

answers: NDQ_002636

answers: Patterns

text: The "Hurry-Scurry Galaxy" in the videogame Super Mario Galaxy has a planet in the similar shape of a rhombicuboctahedron.

text: The "Hurry-Scurry Galaxy" in the videogame

text: Super Mario Galaxy

text: has a planet in the similar shape of a rhombicuboctahedron.

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answers: Our solar system is slowly spinning around our galaxy.

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answers: Our solar system is within one of the spiral arms

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answers: Galaxy

text: In irregular galaxies, open clusters may be found throughout the galaxy, although their concentration is highest where the gas density is highest. Open clusters are not seen in elliptical galaxies: star formation ceased many millions of years ago in ellipticals, and so the open clusters which were originally present have long since dispersed.

text: In

text: irregular galaxies

text: , open clusters may be found throughout the galaxy, although their concentration is highest where the gas density is highest. Open clusters are not seen in

text: elliptical galaxies

text: : star formation ceased many millions of years ago in ellipticals, and so the open clusters which were originally present have long since dispersed.

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answers: open clusters

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answers: star formation ceased

answers: NDQ_002604

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answers: Star formation ceased many millions of years ago in ellipticals

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answers: The solar system is rotating around our galaxy.

answers: NDQ_002627

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answers: galaxies

text: In astronomy, a blue compact dwarf galaxy (BCD galaxy) is a small galaxy which contains large clusters of young, hot, massive stars. These stars, the brightest of which are blue, cause the galaxy itself to appear blue in colour. Most BCD galaxies are also classified as dwarf irregular galaxies or as dwarf lenticular galaxies. Because they are composed of star clusters, BCD galaxies lack a uniform shape. They consume gas intensely, which causes their stars to become very violent when forming.

text: In

text: astronomy

text: , a blue compact dwarf galaxy (BCD galaxy) is a small galaxy which contains large

text: clusters

text: of young, hot, massive

text: star

text: s. These stars, the brightest of which are blue, cause the galaxy itself to appear

text: blue

text: in colour. Most BCD galaxies are also classified as dwarf

text: irregular galaxies

text: or as dwarf

text: lenticular galaxies

text: . Because they are composed of star clusters, BCD galaxies lack a uniform shape. They consume gas intensely, which causes their stars to become very violent when forming.

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text: Around 200,000 light years in diameter, NGC 772 is twice the size of the Milky Way Galaxy, and is surrounded by several satellite galaxies – including the dwarf elliptical, NGC 770 – whose tidal forces on the larger galaxy have likely caused the emergence of a  single elongated outer spiral arm that is much more developed than the others arms. Halton Arp includes NGC 772 in his Atlas of Peculiar Galaxies as Arp 78, where it is described as a "Spiral galaxy with a small high-surface brightness companion".

text: Around 200,000 light years in diameter, NGC 772 is twice the size of the

text: Milky Way Galaxy

text: , and is surrounded by several

text: satellite galaxies

text: – including the dwarf

text: elliptical

text: NGC 770

text: – whose

text: tidal force

text: s on the larger galaxy have likely caused the emergence of a  single elongated outer

text: spiral arm

text: that is much more developed than the others arms.

text: Halton Arp

text: includes NGC 772 in his

text: Atlas of Peculiar Galaxies

text: as

entity_section: Spiral galaxies with small high surface brightness companions

text: Arp 78

text: , where it is described as a "Spiral galaxy with a small high-

text: surface brightness

text: companion".

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answers: Milky Way Galaxy

text: The resulting energy wave broke Replicator Carter and all her brethren into their constituent parts, finally ending the threat of Replicator Carter and her race once and for all although her actions had life-changing consequences for the entire Milky Way galaxy and its people.

text: The resulting energy wave broke Replicator Carter and all her brethren into their constituent parts, finally ending the threat of Replicator Carter and her race once and for all although her actions had life-changing consequences for the entire Milky Way galaxy and its people.

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text: According to the lead programmer of the 16 bit Amiga/Atari ST and the MSX conversions Rob Nicholson, he did not have access to the source code because of contractual issues and had to write them "blind". All he had were the ship shapes and the procedural generation code for the galaxies.

text: According to the lead programmer of the 16 bit Amiga/Atari ST and the MSX conversions Rob Nicholson, he did not have access to the

text: source code

text: because of contractual issues and had to write them "blind". All he had were the ship shapes and the procedural generation code for the galaxies.

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text: NGC 5545 is a spiral galaxy in the northern constellation of Boötes. It is interacting with the spiral galaxy NGC 5544.

text: NGC 5545 is a

text: spiral galaxy

text: in the northern

text: constellation

text: of

text: Boötes

text: . It is interacting with the spiral galaxy

text: NGC 5544

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text: In 2005, astronomers from the University of Wisconsin at Madison and Whitewater determined, on the basis of 400 hours of observation on the Spitzer Space Telescope, that the Milky Way galaxy has a more substantial bar structure across its core than previously recognized.

text: In 2005, astronomers from the

text: University of Wisconsin

text: at

text: Madison

text: and

text: Whitewater

text: determined, on the basis of 400 hours of observation on the Spitzer Space Telescope, that the

text: Milky Way

text: galaxy has a more substantial

text: bar structure

text: across its core than previously recognized.

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text: NGC 3109 is classified as a Magellanic type irregular galaxy, but it may in fact be a small spiral galaxy. If it is a spiral galaxy, it would be the smallest in the Local Group.NGC 3109 has a mass of about 2.3×10 times the mass of the Sun, of which 20% is in the form of neutral hydrogen. It is oriented edge-on from our point of view, and may contain a disk and a halo. The disk appears to be composed of stars of all ages, whereas the halo contains only very old and metal-poor stars. NGC 3109 does not appear to possess a galactic nucleus.

text: NGC 3109 is classified as a

text: Magellanic

text: type

text: irregular galaxy

text: , but it may in fact be a small

text: spiral galaxy

text: . If it is a spiral galaxy, it would be the smallest in the Local Group.NGC 3109 has a mass of about 2.3×10 times the mass of the

text: Sun

text: , of which 20% is in the form of neutral

text: hydrogen

text: . It is oriented edge-on from our point of view, and may contain a

text: disk

text: and a

text: halo

text: . The disk appears to be composed of stars of all ages, whereas the halo contains only very old and

text: metal-poor

text: stars. NGC 3109 does not appear to possess a galactic nucleus.

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answers: The universe has billions of galaxies

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answers: The disk appears to be composed of stars of all ages

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text: The Milky Way galaxy and the nearby Andromeda Galaxy are moving toward each other at about 130 km/s, and—depending upon the lateral movements—the two might collide in about five to six billion years. Although the Milky Way has never collided with a galaxy as large as Andromeda before, evidence of past collisions of the Milky Way with smaller dwarf galaxies is increasing.

text: The Milky Way galaxy and the nearby Andromeda Galaxy are moving toward each other at about 130

text: km/s

text: , and—depending upon the lateral movements—the two might collide in about five to six billion years. Although the Milky Way has never collided with a galaxy as large as Andromeda before, evidence of past collisions of the Milky Way with smaller dwarf galaxies is increasing.

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text: Launched at the 1970 São Paulo Auto Show, the Ford Landau was a full-size car, manufactured in Brazil from 1971 until 1983 by Ford Brasil at their São Paulo facility. It became Ford's flagship in that country. It was based on the U.S. 1966 Ford Galaxie.  It was only offered as a 4-door sedan, although the American version was offered in a wide variety of bodysyles.  After 1976, it gained more differences from the Galaxie and LTD, and featured the newly introduced 302 engine, a lighter 5.0L V8, and its radical restyling clearly resembling the 1965 Lincoln Continental.

text: Launched at the 1970 São Paulo Auto Show, the Ford Landau was a full-size

text: car

text: , manufactured in Brazil from 1971 until 1983 by

text: Ford Brasil

text: at their

text: São Paulo

text: facility. It became Ford's flagship in that country. It was based on the U.S. 1966

text: Ford Galaxie

text: .  It was only offered as a 4-door sedan, although the American version was offered in a wide variety of bodysyles.  After 1976, it gained more differences from the Galaxie and LTD, and featured the newly introduced 302 engine, a lighter 5.0L V8, and its radical restyling clearly resembling the 1965

text: Lincoln Continental

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answers: NDQ_002598

answers: Galaxie

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answers: hundreds of billions

answers: NDQ_002600

answers: galaxie

answers: NDQ_002601

answers: radical restyling

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answers: galaxie

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answers: elliptical

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answers: radical restyling

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answers: stars

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answers: wide variety

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answers: Galaxie

answers: NDQ_002609

answers: billions of stars

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answers: Galaxie

answers: NDQ_002612

answers: Galaxie

answers: NDQ_002615

answers: Galaxie

answers: NDQ_002617

answers: Galaxie

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: galaxie

answers: NDQ_002620

answers: Galaxie

answers: NDQ_002621

answers: Galaxie

answers: NDQ_002622

answers: Galaxie

answers: NDQ_002623

answers: Elliptical galaxie

answers: NDQ_002624

answers: Galaxie

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: Galaxie

answers: NDQ_002628

answers: Galaxie

answers: NDQ_002629

answers: Open star cluster

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answers: full-size

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answers: Spiral

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answers: Galaxie

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answers: Galaxie

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answers: Galaxie

answers: NDQ_002635

answers: Our solar system orbits the central disk of our galaxy

answers: NDQ_002636

answers: Galaxie

text: Other possible members galaxies (galaxies listed in only one or two of the lists from the above references) include the irregular galaxies NGC 5238 and UGC 8508.

text: Other possible members galaxies (galaxies listed in only one or two of the lists from the above references) include the

text: irregular galaxies

text: NGC 5238

text: and

text: UGC 8508

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answers: 1: The answer is not relevant or complete, with substantial shortcomings.

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answers: Galaxies

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answers: stars

answers: NDQ_002600

answers: galaxies

answers: NDQ_002601

answers: only one or two of the lists

answers: NDQ_002602

answers: irregular galaxies

answers: NDQ_002603

answers: irregular galaxies

answers: NDQ_002604

answers: galaxies

answers: NDQ_002605

answers: Galaxies

answers: NDQ_002606

answers: irregular

answers: NDQ_002607

answers: galaxies

answers: NDQ_002609

answers: 4 billion galaxies

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answers: galaxy

answers: NDQ_002612

answers: irregular

answers: NDQ_002615

answers: galaxies

answers: NDQ_002617

answers: UGC 8508

answers: NDQ_002618

answers: The Milky Way is a galaxy.

answers: NDQ_002619

answers: galaxy

answers: NDQ_002620

answers: NGC 5238 and UGC 8508.

answers: NDQ_002621

answers: Galaxies

answers: NDQ_002622

answers: galaxies

answers: NDQ_002623

answers: NGC 5238 and UGC 8508

answers: NDQ_002624

answers: irregular galaxies

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is rotating around our galaxy.

answers: NDQ_002627

answers: galaxies

answers: NDQ_002628

answers: galaxies

answers: NDQ_002629

answers: Open star clusters contain more stars

answers: NDQ_002630

answers: Galaxies are divided into types based on size.

answers: NDQ_002631

answers: Spiral galaxies

answers: NDQ_002632

answers: NGC 5238 and UGC 8508 are dwarf galaxies.

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: Our solar system is within one of the spiral arms of our galaxy.

answers: NDQ_002635

answers: Our solar system orbits the center of our galaxy.

answers: NDQ_002636

answers: NGC 5238 and UGC 8508

text: Edwin Hubble classified spiral galaxies of this type as "SB" (spiral, barred) in his Hubble sequence, and arranged them into sub-categories based on how open the arms of the spiral are. SBa types feature tightly bound arms, while SBc types are at the other extreme and have loosely bound arms. SBb-type galaxies lie in between. SB0 is a barred lenticular galaxy. A new type, SBm, was subsequently created to describe somewhat irregular barred spirals, such as the Magellanic Cloud galaxies, which were once classified as irregular galaxies, but have since been found to contain barred spiral structures. Among other types in Hubble's classifications for the galaxies are: spiral galaxy, elliptical galaxy and irregular galaxy.

text: Edwin Hubble

text: classified spiral galaxies of this type as "SB" (spiral, barred) in his

text: Hubble sequence

text: , and arranged them into sub-categories based on how open the arms of the spiral are. SBa types feature tightly bound arms, while SBc types are at the other extreme and have loosely bound arms. SBb-type galaxies lie in between. SB0 is a barred

text: lenticular galaxy

text: . A new type, SBm, was subsequently created to describe somewhat

text: irregular

text: barred spirals, such as the

text: Magellanic Cloud galaxies

text: , which were once classified as irregular galaxies, but have since been found to contain barred spiral structures. Among other types in Hubble's classifications for the galaxies are:

text: spiral galaxy

text: elliptical galaxy

text: and

text: irregular galaxy

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answers: Spiral galaxy

text: In 1932, Jan Hendrik Oort became the first to report that measurements of the stars in the Solar neighborhood moved faster than expected when a mass distribution based upon visible matter was assumed, but this measurement was later determined to be essentially erroneous. In 1939, Horace Babcock reported in his PhD thesis measurements of the rotation curve for Andromeda which suggested that the mass-to-luminosity ratio increases radially. He attributed that to either the absorption of light within the galaxy or to modified dynamics in the outer portions of the spiral and not to any form of missing matter. In 1959, Louise Volders demonstrated that spiral galaxy M33 does not spin as expected according to Keplerian dynamics. In the late 1960s and early 1970s, Vera Rubin, an astronomer at the Department of Terrestrial Magnetism at the Carnegie Institution of Washington worked with a new sensitive spectrograph that could measure the velocity curve of edge-on spiral galaxies to a greater degree of accuracy than had ever before been achieved. Together with fellow staff-member Kent Ford, Rubin announced at a 1975 meeting of the American Astronomical Society the discovery that most stars in spiral galaxies orbit at roughly the same speed, and that this implied that galaxy masses grow approximately linearly with radius well beyond the location of most of the stars (the galactic bulge).  Rubin presented her results in an influential paper in 1980. These were the first robust results to suggest that either Newtonian gravity does not apply universally or that, conservatively, upwards of 50% of the mass of galaxies was contained in the relatively dark galactic halo. Although initially met with skepticism,  Rubin's results have been confirmed over the subsequent decades.

text: In 1932,

text: Jan Hendrik Oort

text: became the first to report that measurements of the stars in the

text: Solar neighborhood

text: moved faster than expected when a mass distribution based upon visible matter was assumed, but this measurement was later determined to be essentially erroneous. In 1939,

text: Horace Babcock

text: reported in his PhD thesis measurements of the rotation curve for Andromeda which suggested that the mass-to-luminosity ratio increases radially. He attributed that to either the absorption of light within the galaxy or to modified dynamics in the outer portions of the spiral and not to any form of missing matter. In 1959, Louise Volders demonstrated that spiral galaxy

text: does not spin as expected according to

text: Keplerian dynamics

text: . In the late 1960s and early 1970s,

text: Vera Rubin

text: , an astronomer at the Department of Terrestrial Magnetism at the

text: Carnegie Institution of Washington

text: worked with a new sensitive

text: spectrograph

text: that could measure the velocity curve of edge-on

text: spiral galaxies

text: to a greater degree of accuracy than had ever before been achieved. Together with fellow staff-member

text: Kent Ford

text: , Rubin announced at a 1975 meeting of the

text: American Astronomical Society

text: the discovery that most

text: star

text: s in

text: spiral galaxies

text: orbit at roughly the same speed, and that this implied that galaxy masses grow approximately linearly with radius well beyond the location of most of the stars (the

text: galactic bulge

text: ).  Rubin presented her results in an influential paper in 1980. These were the first robust results to suggest that either

text: Newtonian gravity

text: does not apply universally or that, conservatively, upwards of 50% of the mass of galaxies was contained in the relatively dark galactic halo. Although initially met with skepticism,  Rubin's results have been confirmed over the subsequent decades.

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answers: 2: The answer has limited relevance and completeness, with noticeable gaps or inaccuracy.

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answers: galaxies

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answers: upwards of 50%

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answers: dark galactic halo

answers: NDQ_002601

answers: the galactic bulge

answers: NDQ_002602

answers: edge-on spiral

answers: NDQ_002603

answers: gravitational force

answers: NDQ_002604

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answers: orbit at roughly the same speed

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answers: halo

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answers: 50% of the mass of galaxies

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answers: galaxy masses grow approximately linearly with radius well beyond the location of most of the stars

answers: NDQ_002624

answers: galactic halo

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The discovery that most stars in spiral galaxies orbit at roughly the same speed

answers: NDQ_002627

answers: upwards of 50% of the mass of galaxies

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answers: galaxy

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answers: open star clusters

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answers: dwarf galaxies are often found near larger galaxies

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answers: The Solar neighborhood

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answers: Andromeda

text: Messier 74 (also known as NGC 628) is a  spiral galaxy in the constellation Pisces. It is at a distance of about 32 million light-years away from Earth. The galaxy contains two clearly defined spiral arms and is therefore used as an archetypal example of a grand design spiral galaxy.  The galaxy's low surface brightness makes it the most difficult Messier object for amateur astronomers to observe.  However, the relatively large angular size of the galaxy and the galaxy's face-on orientation make it an ideal object for professional astronomers who want to study spiral arm structure and spiral density waves. It is estimated that M74 is home to about 100 billion stars.

text: Messier 74 (also known as NGC 628) is a

text: spiral galaxy

text: in the

text: constellation

text: Pisces

text: . It is at a distance of about 32 million light-years away from Earth. The galaxy contains two clearly defined

text: spiral arm

text: s and is therefore used as an archetypal example of a

text: grand design spiral galaxy

text: .  The galaxy's low surface brightness makes it the most difficult

text: Messier object

text: for amateur astronomers to observe.  However, the relatively large angular size of the galaxy and the galaxy's face-on orientation make it an ideal object for professional astronomers who want to study

text: spiral arm

text: structure and

text: spiral density waves

text: . It is estimated that M74 is home to about 100 billion stars.

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answers: Messier 74

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answers: The Milky Way Galaxy

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answers: 32 million light-years away

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answers: It is estimated that M74 is home to about 100 billion stars

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answers: star cluster

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answers: It is estimated that M74 is home to about 100 billion stars

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answers: The galaxy contains two clearly defined spiral arms

text: Gestaltzerfall (German for "shape decomposition") refers to a type of visual agnosia and is a psychological phenomenon where delays in recognition are observed when a complex shape is stared at for a while as the shape seems to decompose into its constituting parts. With regards to kanji, a study has shown that delays are most significant when the characters are of the same size. When characters to recognize are of different sizes, delays are observed only when they are of different patterns.

text: Gestaltzerfall (German for "shape decomposition") refers to a type of

text: visual agnosia

text: and is a

text: psychological

text: phenomenon where delays in recognition are observed when a complex shape is stared at for a while as the shape seems to decompose into its constituting parts. With regards to

text: kanji

text: , a study has shown that delays are most significant when the characters are of the same size. When characters to recognize are of different sizes, delays are observed only when they are of different patterns.

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answers: unanswerable

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answers: It is not possible to tell

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answers: Milky Way Galaxy

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answers: It revolves around our galaxy.

answers: NDQ_002627

answers: galaxies

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answers: Star cluster

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answers: It seems to decompose into its constituting parts

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answers: galaxies

answers: NDQ_002634

answers: galaxy

answers: NDQ_002635

answers: Our solar system orbits the central disk of our galaxy

answers: NDQ_002636

answers: Gestaltzerfall

text: Shapes of physical objects are equal if the subsets of space these objects occupy satisfy the definition above. In particular, the shape does not depend on the size and placement in space of the object. For instance, a "

text: Shapes of physical objects are equal if the subsets of space these objects occupy satisfy the definition above. In particular, the shape does not depend on the size and placement in space of the object. For instance, a "

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answers: 1"

answers: NDQ_002636

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answers: NDQ_002598

answers: star "

answers: NDQ_002599

answers: galaxy

answers: NDQ_002600

answers: galaxies"

answers: NDQ_002601

answers: shape does not depend on the size

answers: NDQ_002602

answers: galaxy "

answers: NDQ_002603

answers: elliptical galaxy

answers: NDQ_002604

answers: shape "

answers: NDQ_002605

answers: open cluster"

answers: NDQ_002606

answers: shapeless "

answers: NDQ_002607

answers: globular cluster" is a cluster of stars

answers: NDQ_002609

answers: galaxies

answers: NDQ_002610

answers: galaxy "

answers: NDQ_002612

answers: globular

answers: NDQ_002615

answers: star cluster

answers: NDQ_002617

answers: galaxy

answers: NDQ_002618

answers: galaxy "

answers: NDQ_002619

answers: subset

answers: NDQ_002620

answers: dwarf galaxies"

answers: NDQ_002621

answers: binary star"

answers: NDQ_002622

answers: star cluster

answers: NDQ_002623

answers: elliptical " galaxy

answers: NDQ_002624

answers: globular

answers: NDQ_002625

answers: Milky Way Galaxy"

answers: NDQ_002626

answers: galaxy" is a galaxy.

answers: NDQ_002627

answers: galaxies "

answers: NDQ_002628

answers: star cluster "

answers: NDQ_002629

answers: globular star cluster"

answers: NDQ_002630

answers: galaxies"

answers: NDQ_002631

answers: elliptical galaxies"

answers: NDQ_002632

answers: dwarf galaxies " are often found near larger galaxies

answers: NDQ_002633

answers: galaxy "

answers: NDQ_002634

answers: galaxy "

answers: NDQ_002635

answers: solar system " orbits our galaxy.

answers: NDQ_002636

answers: galaxy "

text: X-shaped (or "winged") radio galaxies are a class of extragalactic radio source that exhibit two, low-surface-brightness radio lobes (the "wings") oriented at an angle to the active, or high-surface-brightness, lobes. Both sets of lobes pass symmetrically through the center of the elliptical galaxy that is the source of the lobes, giving the radio galaxy an X-shaped morphology as seen on radio maps (see figure).

text: X-shaped (or "winged") radio galaxies are a class of extragalactic

text: radio source

text: that exhibit two, low-surface-brightness radio lobes (the "wings") oriented at an angle to the active, or high-surface-brightness, lobes. Both sets of lobes pass symmetrically through the center of the

text: elliptical galaxy

text: that is the source of the lobes, giving the

text: radio galaxy

text: an X-shaped morphology as seen on radio maps (see figure).

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answers: X-shaped

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answers: 4

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answers: 4

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answers: NDQ_002626

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answers: 4

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answers: 2

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answers: NDQ_002635

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answers: NDQ_002636

answers: 0

answers: NDQ_002598

answers: radio galaxies

answers: NDQ_002599

answers: galaxy

answers: NDQ_002600

answers: radio lobes

answers: NDQ_002601

answers: X-shaped

answers: NDQ_002602

answers: elliptical

answers: NDQ_002603

answers: low-surface-brightness

answers: NDQ_002604

answers: X-shaped

answers: NDQ_002605

answers: active

answers: NDQ_002606

answers: elliptical

answers: NDQ_002607

answers: radio galaxies

answers: NDQ_002609

answers: billions of stars

answers: NDQ_002610

answers: X-shaped

answers: NDQ_002612

answers: Ellipsical galaxy

answers: NDQ_002615

answers: galaxy

answers: NDQ_002617

answers: elliptical

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: extragalactic

answers: NDQ_002620

answers: elliptical

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxy

answers: NDQ_002623

answers: low-surface-brightness

answers: NDQ_002624

answers: radio galaxy

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: It's impossible to say

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: elliptical

answers: NDQ_002631

answers: elliptical

answers: NDQ_002632

answers: Dwarf galaxies are often found near larger galaxies

answers: NDQ_002633

answers: galaxy

answers: NDQ_002634

answers: elliptical galaxy

answers: NDQ_002635

answers: elliptical galaxy

answers: NDQ_002636

answers: elliptical

text: Circinus also houses ESO 97-G13, commonly known as the Circinus Galaxy. Discovered in 1977, it is a relatively unobscured galaxy (magnitude 10.6), which is unusual for galaxies located in constellations near the Milky Way, since their dim light is obscured by gas and dust. This oblong spiral galaxy with 6.9 by 3.0 arcminutes and 26,000 light-years in diameter, is located 13 million light-years away from Earth and lies 4 degrees off the galactic plane. It is the closest Seyfert galaxy to the Milky Way, and therefore hosts an active galactic nucleus.

text: Circinus also houses ESO 97-G13, commonly known as the

text: Circinus Galaxy

text: . Discovered in 1977, it is a relatively unobscured galaxy (magnitude 10.6), which is unusual for galaxies located in constellations near the

text: Milky Way

text: , since their dim light is obscured by gas and dust. This oblong

text: spiral galaxy

text: with 6.9 by 3.0 arcminutes and 26,000 light-years in diameter, is located 13 million light-years away from Earth and lies 4 degrees off the

text: galactic plane

text: . It is the closest

text: Seyfert galaxy

text: to the Milky Way, and therefore hosts an

text: active galactic nucleus

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answers: Milky Way

text: In 1963, Dick Brannan set the NHRA Super/Stock National record at 12.42 on a hot July day. In the biggest race of the year, the INDY Nationals, Ed Martin's lightweight Galaxie lost the Super Stock trophy run to John Barker's Dodge but at the teardown, the Dodge was found to have an illegal cam. In drag racing, the 427 Ford Galaxie was a winner in three consecutive National Events: the '64 Indy Nationals, the 1965 WinterNationals and the 1965 Indy Nationals.  It was Mike Schmitt driving the Desert Motors Galaxie to the AA/SA Class win at the 1964 Indy Nationals. At the 1965 Winternationals it was a clean sweep as Doug Butler's four-speed took the win in AA/S with a 12.77 @ 114.21 and Bill Hanyon won on the automatic side with a 12.24 @ 117.95. Additionally, Bud Schellenberger's "Double A Stock" 1964 Galaxie was the 1965 Indy Nationals Top Stock Eliminator with a 12.16 @ 114.21. The Shelby Super Snake top fuel dragster, powered by a 427 supercharged SOHC, became the first car in NHRA competition to break the six-second quarter-mile time barrier.  It was the winner of the 1966 NHRA Spring Nationals. In every decade since, the FE has held drag-racing records. In 2011, the new decade opens with the NHRA SS/F (class rules include stock compression ratio, stock valve sizes, stock carb sizing and other OEM-type equipment limitations) national record:  the quartermile in 9.29 seconds, with a closing speed of 143.63 mph.

text: OEM

text: -type equipment limitations) national record:  the quartermile in 9.29 seconds, with a closing speed of 143.63 mph.

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answers: NDQ_002626

answers: Our solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: galaxies

answers: NDQ_002628

answers: Star cluster

answers: NDQ_002629

answers: Open star cluster

answers: NDQ_002630

answers: lightweight

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answers: Spiral

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answers: dwarf galaxies

answers: NDQ_002633

answers: Galaxie

answers: NDQ_002634

answers: galaxy

answers: NDQ_002635

answers: Earth orbits the central disk of our galaxy

answers: NDQ_002636

answers: Galaxie

text: NGC 93 (PGC 1412) is an interacting spiral galaxy located in Andromeda constellation. The galaxy is 100 thousand light-years across and was discovered by R. J. Mitchell in 1854. The galaxy is currently interacting with NGC 90, a nearby large spiral galaxy.

text: NGC 93 (PGC 1412) is an interacting

text: spiral galaxy

text: located in

text: Andromeda constellation

text: . The

text: galaxy

text: is 100 thousand light-years across and was discovered by R. J. Mitchell in 1854. The galaxy is currently interacting with

text: NGC 90

text: , a nearby large spiral galaxy.

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answers: NDQ_002598

answers: spiral galaxy

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answers: large spiral galaxy

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answers: NDQ_002617

answers: large spiral galaxy

answers: NDQ_002618

answers: Andromeda constellation

answers: NDQ_002619

answers: constellation

answers: NDQ_002620

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answers: NDQ_002623

answers: Spiral

answers: NDQ_002624

answers: interacting

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The galaxy is currently interacting with NGC 90

answers: NDQ_002627

answers: 100 thousand light-years across

answers: NDQ_002628

answers: galaxy

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answers: Open star clusters

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answers: large

answers: NDQ_002631

answers: Spiral galaxies

answers: NDQ_002632

answers: nearby large spiral galaxy

answers: NDQ_002633

answers: 100 thousand light-years

answers: NDQ_002634

answers: NGC 93

answers: NDQ_002635

answers: 100 thousand light-years

answers: NDQ_002636

answers: Andromeda

text: The archetype of such a colliding-wind binary system is WR140 (HD 193793), which consists of a 20 solar mass () Wolf-Rayet star orbiting about a , spectral class O4-5 main sequence star every 7.9 years. The high orbital eccentricity of the pair allows astronomers to observe changes the colliding winds as their separation varies. Another prominent example of a colliding-wind binary is thought to be Eta Carinae, one of the most luminous objects in the Milky Way galaxy. The first colliding-wind binary to be detected in the X-ray band outsidethe Milky Way galaxy was HD 5980, located in the Small Magellanic Cloud.

text: The archetype of such a colliding-wind binary system is

text: (HD 193793), which consists of a 20

text: solar mass

text: Wolf-Rayet star

text: orbiting about a ,

text: spectral class

text: O4-5 main sequence star

text: every 7.9 years. The high

text: orbital eccentricity

text: of the pair allows astronomers to observe changes the colliding winds as their separation varies. Another prominent example of a colliding-wind binary is thought to be

text: Eta Carinae

text: , one of the most luminous objects in the

text: Milky Way

text: galaxy. The first colliding-wind binary to be detected in the X-ray band outsidethe Milky Way galaxy was

text: HD 5980

text: , located in the

text: Small Magellanic Cloud

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answers: Small Magellanic Cloud

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answers: colliding wind binary

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answers: high orbital eccentricity

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answers: Milky Way galaxy

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answers: colliding-wind binary

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answers: colliding-wind binary

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answers: Small Magellanic Cloud

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answers: Small Magellanic Cloud

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answers: 20 solar mass

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answers: Milky Way galaxy

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answers: Small Magellanic Cloud

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answers: Milky Way galaxy

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: Small Magellanic Cloud

answers: NDQ_002623

answers: Wolf-Rayet star

answers: NDQ_002624

answers: Small Magellanic Cloud

answers: NDQ_002625

answers: Milky Way galaxy

answers: NDQ_002626

answers: orbiting about a main sequence star every 7.9 years

answers: NDQ_002627

answers: The universe has billions of galaxies

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answers: Small Magellanic Cloud

answers: NDQ_002629

answers: Open star clusters

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answers: solar mass

answers: NDQ_002631

answers: colliding-wind binary

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answers: Small Magellanic Cloud

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answers: The Small Magellanic Cloud

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answers: Milky Way galaxy

answers: NDQ_002635

answers: The Milky Way galaxy

answers: NDQ_002636

answers: Milky Way

text: The horror-based story, which ties into the Shadow/Vorlon plotline, centers on the return of an ancient and overwhelming alien force which had once attempted to destroy life in the Milky Way Galaxy.

text: The horror-based story, which ties into the Shadow/Vorlon plotline, centers on the return of an ancient and overwhelming alien force which had once attempted to destroy life in the

text: Milky Way Galaxy

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answers: Milky Way Galaxy

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answers: Milky Way Galaxy

text: Canes Venatici contains five Messier objects, including four galaxies. One of the more significant galaxies in Canes Venatici is the Whirlpool Galaxy (M51, NGC 5194) and NGC 5195, a small barred spiral galaxy that is seen face on. This was the first galaxy recognised as having a spiral structure, this structure being first observed by Lord Rosse in 1845. It is a face-on spiral galaxy 37 million light-years from Earth. Widely considered to be one of the most beautiful galaxies visible, M51 has many star-forming regions and nebulae in its arms, coloring them pink and blue in contrast to the older yellow core. M51 has a smaller companion, NGC 5195, that has very few star-forming regions and thus appears yellow. It is passing behind M51 and may be the cause of the larger galaxy's prodigious star formation.

text: Canes Venatici contains five

text: Messier object

text: s, including four

text: galaxies

text: . One of the more significant galaxies in Canes Venatici is the

text: Whirlpool Galaxy

text: (M51, NGC 5194) and

text: NGC 5195

text: , a small barred

text: spiral galaxy

text: that is seen face on. This was the first galaxy recognised as having a spiral structure, this structure being first observed by

text: Lord Rosse

text: in 1845. It is a face-on spiral galaxy 37 million light-years from Earth. Widely considered to be one of the most beautiful galaxies visible, M51 has many

text: star-forming regions

text: and

text: nebula

text: e in its arms, coloring them pink and blue in contrast to the older yellow core. M51 has a smaller companion, NGC 5195, that has very few star-forming regions and thus appears yellow. It is passing behind M51 and may be the cause of the larger galaxy's prodigious star formation.

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answers: barred

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: It is passing behind M51

answers: NDQ_002627

answers: It is a face-on spiral galaxy

answers: NDQ_002628

answers: star clusters

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: barred spiral galaxy

answers: NDQ_002631

answers: Spiral

answers: NDQ_002632

answers: smaller companion

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: Canes Venatici

answers: NDQ_002635

answers: The Whirlpool Galaxy

answers: NDQ_002636

answers: face-on spiral galaxy

text: The rotational dynamics of galaxies are well characterized by their position on the Tully–Fisher relation, which shows that for spiral galaxies the rotational velocity is uniquely related to its total luminosity. A consistent way to predict the rotational velocity of a spiral galaxy is to measure its bolometric luminosity and then read its rotation rate from its location on the Tully–Fisher diagram. Conversely, knowing the rotational velocity of a spiral galaxy gives its luminosity. Thus the magnitude of the galaxy rotation is related to the galaxy's visible mass.

text: The rotational dynamics of galaxies are well characterized by their position on the

text: Tully–Fisher relation

text: , which shows that for spiral galaxies the rotational velocity is uniquely related to its total luminosity. A consistent way to predict the rotational velocity of a spiral galaxy is to measure its

text: bolometric luminosity

text: and then read its rotation rate from its location on the Tully–Fisher diagram. Conversely, knowing the rotational velocity of a spiral galaxy gives its luminosity. Thus the magnitude of the galaxy rotation is related to the galaxy's visible mass.

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answers: 4

answers: NDQ_002598

answers: galaxies

answers: NDQ_002599

answers: total luminosity

answers: NDQ_002600

answers: luminosity

answers: NDQ_002601

answers: Tully–Fisher diagram

answers: NDQ_002602

answers: spiral

answers: NDQ_002603

answers: luminosity

answers: NDQ_002604

answers: luminosity

answers: NDQ_002605

answers: luminosity

answers: NDQ_002606

answers: spiral

answers: NDQ_002607

answers: galaxies

answers: NDQ_002609

answers: visible mass

answers: NDQ_002610

answers: galaxies

answers: NDQ_002612

answers: spiral

answers: NDQ_002615

answers: galaxy

answers: NDQ_002617

answers: spiral galaxy

answers: NDQ_002618

answers: luminosity

answers: NDQ_002619

answers: dwarf galaxy

answers: NDQ_002620

answers: spiral galaxies

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxy

answers: NDQ_002623

answers: Spiral galaxies

answers: NDQ_002624

answers: galaxy's visible mass

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: It rotates around our galaxy.

answers: NDQ_002627

answers: galaxies

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: open star clusters

answers: NDQ_002630

answers: spiral galaxies

answers: NDQ_002631

answers: Spiral galaxies

answers: NDQ_002632

answers: Tully–Fisher relation

answers: NDQ_002633

answers: galaxy's visible mass

answers: NDQ_002634

answers: galaxy

answers: NDQ_002635

answers: Galaxies

answers: NDQ_002636

answers: Tully–Fisher relation

text: A pinwheel-shaped disk, rotating in a direction opposite to that of the galaxy, is found deep inside NGC 7252: it resembles a face-on spiral galaxy, yet it is only 10,000 light years across. It is believed that this pinwheel-shaped structure is a remnant of a collision between two galaxies. Within a few billion years, NGC 7252 will look like an elliptical galaxy with a small inner disk due to the exhaustion of the gases in the galaxy.

text: A pinwheel-shaped disk, rotating in a direction opposite to that of the galaxy, is found deep inside NGC 7252: it resembles a face-on spiral galaxy, yet it is only 10,000 light years across. It is believed that this pinwheel-shaped structure is a remnant of a collision between two galaxies. Within a few billion years, NGC 7252 will look like an elliptical galaxy with a small inner disk due to the exhaustion of the gases in the galaxy.

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answers: NDQ_002598

answers: star clusters

answers: NDQ_002599

answers: billion years

answers: NDQ_002600

answers: gases

answers: NDQ_002601

answers: exhaustion of the gases

answers: NDQ_002602

answers: face-on spiral galaxy

answers: NDQ_002603

answers: exhaustion

answers: NDQ_002604

answers: a small inner disk

answers: NDQ_002605

answers: galaxy

answers: NDQ_002606

answers: elliptical

answers: NDQ_002607

answers: NGC 7252

answers: NDQ_002609

answers: 1 billion stars

answers: NDQ_002610

answers: collision between two galaxies

answers: NDQ_002612

answers: face-on spiral

answers: NDQ_002615

answers: NGC 7252

answers: NDQ_002617

answers: elliptical galaxy

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: disk

answers: NDQ_002620

answers: face-on spiral

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxy

answers: NDQ_002623

answers: elliptical galaxy

answers: NDQ_002624

answers: pinwheel-shaped

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: It resembles a face-on spiral galaxy

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: NGC 7252

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: face-on spiral galaxy

answers: NDQ_002631

answers: elliptical

answers: NDQ_002632

answers: NGC 7252

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: NGC 7252

answers: NDQ_002635

answers: galaxy

answers: NDQ_002636

answers: face-on spiral galaxy

text: A majority of spiral galaxies, including our own Milky Way galaxy, have a linear, bar-shaped band of stars that extends outward to either side of the core, then merges into the spiral arm structure. In the Hubble classification scheme, these are designated by an SB, followed by a lower-case letter (a, b or c) that indicates the form of the spiral arms (in the same manner as the categorization of normal spiral galaxies). Bars are thought to be temporary structures that can occur as a result of a density wave radiating outward from the core, or else due to a tidal interaction with another galaxy. Many barred spiral galaxies are active, possibly as a result of gas being channeled into the core along the arms.

text: A majority of spiral galaxies, including our own

text: Milky Way

text: galaxy, have a linear, bar-shaped band of stars that extends outward to either side of the core, then merges into the spiral arm structure. In the Hubble classification scheme, these are designated by an SB, followed by a lower-case letter (a, b or c) that indicates the form of the spiral arms (in the same manner as the categorization of normal spiral galaxies). Bars are thought to be temporary structures that can occur as a result of a density wave radiating outward from the core, or else due to a

text: tidal interaction

text: with another galaxy. Many barred spiral galaxies are active, possibly as a result of gas being channeled into the core along the arms.

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answers: barred

answers: NDQ_002599

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answers: NDQ_002600

answers: stars

answers: NDQ_002601

answers: bar-shaped band of stars

answers: NDQ_002602

answers: Spiral

answers: NDQ_002603

answers: bar-shaped band of stars

answers: NDQ_002604

answers: bar-shaped band of stars

answers: NDQ_002605

answers: bar

answers: NDQ_002606

answers: barred

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answers: bar-shaped band of stars

answers: NDQ_002609

answers: stars

answers: NDQ_002610

answers: density wave

answers: NDQ_002612

answers: Milky Way galaxy

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answers: Milky Way galaxy

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answers: galaxy

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answers: Milky Way galaxy

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answers: galaxy

answers: NDQ_002622

answers: Milky Way galaxy

answers: NDQ_002623

answers: The Milky Way galaxy

answers: NDQ_002624

answers: Milky Way

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answers: Milky Way galaxy

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answers: Milky Way galaxy

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answers: open star clusters

answers: NDQ_002630

answers: The Hubble classification scheme

answers: NDQ_002631

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answers: NDQ_002632

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answers: Milky Way galaxy

answers: NDQ_002634

answers: Milky Way galaxy

answers: NDQ_002635

answers: Milky Way galaxy

answers: NDQ_002636

answers: Milky Way galaxy

text: The Sculptor Galaxy, also known as the Silver Coin or Silver Dollar Galaxy, NGC 253, is an intermediate spiral galaxy in the constellation Sculptor.  The Sculptor Galaxy is a starburst galaxy, which means that it is currently undergoing a period of intense star formation.

text: The Sculptor Galaxy, also known as the Silver Coin or Silver Dollar Galaxy, NGC 253, is an

text: intermediate spiral galaxy

text: in the

text: constellation

text: Sculptor

text: .  The Sculptor Galaxy is a

text: starburst galaxy

text: , which means that it is currently undergoing a period of intense

text: star formation

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answers: NDQ_002598

answers: starburst galaxy

answers: NDQ_002599

answers: galaxy

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answers: Stars

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answers: Sculptor

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answers: intermediate spiral galaxy

answers: NDQ_002603

answers: elliptical

answers: NDQ_002604

answers: star formation

answers: NDQ_002605

answers: starburst

answers: NDQ_002606

answers: intermediate

answers: NDQ_002607

answers: Sculptor Galaxy

answers: NDQ_002609

answers: 1 billion stars

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answers: starburst galaxy

answers: NDQ_002612

answers: spiral

answers: NDQ_002615

answers: The Sculptor Galaxy

answers: NDQ_002617

answers: Sculptor Galaxy

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: constellation

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answers: intermediate spiral galaxy

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: The Sculptor Galaxy

answers: NDQ_002623

answers: Sculptor Galaxy

answers: NDQ_002624

answers: starburst galaxy

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The Sculptor Galaxy

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: Star clusters

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: intermediate

answers: NDQ_002631

answers: The Sculptor Galaxy

answers: NDQ_002632

answers: The Sculptor Galaxy

answers: NDQ_002633

answers: The Sculptor Galaxy

answers: NDQ_002634

answers: intermediate spiral galaxy

answers: NDQ_002635

answers: The Sculptor Galaxy

answers: NDQ_002636

answers: intermediate spiral galaxy

text: The dwarf galaxy problem, also known as the missing satellites problem, arises from numerical cosmological simulations that predict the evolution of the distribution of matter in the universe. Dark matter seems to cluster hierarchically and in ever increasing number counts for smaller-and-smaller-sized halos. However, although there seem to be enough observed normal-sized galaxies to account for this distribution, the number of dwarf galaxies is orders of magnitude lower than expected from simulation. For comparison, there were observed to be around 38 dwarf galaxies in the Local Group, and only around 11 orbiting the Milky Way, (for a detailed and more up to date list see List of Milky Way's satellite galaxies) yet one dark matter simulation predicted around 500 Milky Way dwarf satellites.

text: The dwarf galaxy problem, also known as the missing satellites problem, arises from numerical

text: cosmological

text: simulation

text: s that predict the evolution of the distribution of

text: matter

text: in the

text: universe

text: Dark matter

text: seems to cluster hierarchically and in ever increasing number counts for smaller-and-smaller-sized

text: halos

text: . However, although there seem to be enough observed normal-sized

text: galaxies

text: to account for this distribution, the number of

text: dwarf galaxies

text: is

text: orders of magnitude

text: lower than expected from simulation. For comparison, there were observed to be around 38 dwarf galaxies in the

text: Local Group

text: , and only around 11 orbiting the

text: Milky Way

text: , (for a detailed and more up to date list see

text: List of Milky Way's satellite galaxies

text: ) yet one dark matter simulation predicted around 500 Milky Way dwarf satellites.

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answers: NDQ_002634

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answers: NDQ_002635

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answers: NDQ_002636

answers: 4

answers: NDQ_002598

answers: dwarf galaxies

answers: NDQ_002599

answers: 500

answers: NDQ_002600

answers: Dark matter

answers: NDQ_002601

answers: Dark matter seems to cluster hierarchically

answers: NDQ_002602

answers: dwarf galaxies

answers: NDQ_002603

answers: Dark matter seems to cluster hierarchically

answers: NDQ_002604

answers: halos

answers: NDQ_002605

answers: Dark matter

answers: NDQ_002606

answers: dwarf

answers: NDQ_002607

answers: Dark matter

answers: NDQ_002609

answers: 11

answers: NDQ_002610

answers: Dark matter

answers: NDQ_002612

answers: orbiting

answers: NDQ_002615

answers: dwarf galaxy

answers: NDQ_002617

answers: Milky Way

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: dwarf galaxies

answers: NDQ_002620

answers: normal-sized galaxies

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: dwarf galaxy

answers: NDQ_002623

answers: The dwarf galaxy problem

answers: NDQ_002624

answers: dwarf galaxy

answers: NDQ_002625

answers: Milky Way

answers: NDQ_002626

answers: orbiting the Milky Way

answers: NDQ_002627

answers: It seems to cluster hierarchically

answers: NDQ_002628

answers: Galaxies

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: dwarf galaxy

answers: NDQ_002631

answers: The dwarf galaxy problem

answers: NDQ_002632

answers: Dark matter seems to cluster hierarchically

answers: NDQ_002633

answers: The dwarf galaxy problem

answers: NDQ_002634

answers: Milky Way

answers: NDQ_002635

answers: Milky Way

answers: NDQ_002636

answers: Milky Way

text: The biggest problem with Arp's analysis is that today there are hundreds of thousands of quasars with known redshifts discovered by various sky surveys. The vast majority of these quasars are not correlated in any way with nearby AGN. Indeed, with improved observing techniques, a number of host galaxies have been observed around quasars which indicates that those quasars at least really are at cosmological distances and are not the kind of objects Arp proposes. Arp's analysis, according to most scientists, suffers from being based on small number statistics and hunting for peculiar coincidences and odd associations. Unbiased samples of sources, taken from numerous galaxy surveys of the sky show none of the proposed 'irregularities', nor that any statistically significant correlations exist.

text: The biggest problem with Arp's analysis is that today there are hundreds of thousands of quasars with known redshifts discovered by various

text: sky surveys

text: . The vast majority of these quasars are not correlated in any way with nearby AGN. Indeed, with improved observing techniques, a number of host galaxies have been observed around quasars which indicates that those quasars at least really are at

text: cosmological distances

text: and are not the kind of objects Arp proposes. Arp's analysis, according to most scientists, suffers from being based on

text: small number statistics

text: and hunting for peculiar coincidences and odd associations. Unbiased samples of sources, taken from numerous

text: galaxy survey

text: s of the sky show none of the proposed 'irregularities', nor that any

text: statistically significant

text: correlations exist.

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answers: NDQ_002598

answers: AGN

answers: NDQ_002599

answers: hundreds of thousands

answers: NDQ_002600

answers: AGN

answers: NDQ_002601

answers: redshifts

answers: NDQ_002602

answers: AGN

answers: NDQ_002603

answers: cosmological distances

answers: NDQ_002604

answers: redshifts

answers: NDQ_002605

answers: AGN

answers: NDQ_002606

answers: AGN

answers: NDQ_002607

answers: AGN

answers: NDQ_002609

answers: millions of galaxies

answers: NDQ_002610

answers: AGN

answers: NDQ_002612

answers: AGN

answers: NDQ_002615

answers: AGN

answers: NDQ_002617

answers: AGN

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: AGN

answers: NDQ_002620

answers: AGN

answers: NDQ_002621

answers: AGN

answers: NDQ_002622

answers: AGN

answers: NDQ_002623

answers: Arp's analysis

answers: NDQ_002624

answers: AGN

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: quasars are not correlated in any way with nearby AGN

answers: NDQ_002627

answers: galaxy surveys of the sky

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answers: NDQ_002629

answers: Open star clusters

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answers: spiral galaxies

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answers: host galaxies

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answers: galaxies

text: The central elliptical cD galaxy of this cluster is undergoing a massive starburst, the highest recorded in a middle of a galaxy cluster, although other galaxies at higher redshifts have a higher starburst rate (see Baby Boom Galaxy).Observations by a variety of telescopes including the GALEX and Herschel space telescopes shows that it has been converting material to stars at an exceptionally high rate of 740  per year. This is considerably higher than that of NGC 1275 A, the central galaxy of the Perseus Cluster, where stars are formed at a rate around 20 times lower, or the one per year rate of star formation in the Milky Way.

text: The central elliptical cD galaxy of this cluster is undergoing a massive starburst, the highest recorded in a middle of a galaxy cluster, although other galaxies at higher redshifts have a higher starburst rate (see

text: Baby Boom Galaxy

text: ).Observations by a variety of telescopes including the

text: GALEX

text: and

text: Herschel

text: space telescopes shows that it has been converting material to stars at an exceptionally high rate of 740  per year. This is considerably higher than that of

text: NGC 1275

text: A, the central galaxy of the

text: Perseus Cluster

text: , where stars are formed at a rate around 20 times lower, or the one per year rate of star formation in the

text: Milky Way

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answers: NDQ_002604

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answers: cD

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answers: NDQ_002612

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answers: NDQ_002626

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text: This complex galaxy is inclined by an angle of about 53° to the line of sight from the Earth, which is oriented at a position angle of 172°. It is categorized as a double-barred spiral galaxy with a small inner bulge through the core along with an outer bulge. The nucleus displays a weak level of activity of the LINER2 type. Variations in ultraviolet emission from the core suggest the presence of a supermassive black hole. Estimates for the mass of this object range from  to  times the mass of the Sun.

text: This complex galaxy is inclined by an angle of about 53° to the line of sight from the

text: Earth

text: , which is oriented at a

text: position angle

text: of 172°. It is categorized as a double-barred spiral galaxy with a small inner bulge through the core along with an outer bulge. The nucleus displays a weak level of activity of the

entity_name: Low-ionization nuclear emission-line region

text: LINER

text: 2 type. Variations in

text: ultraviolet

text: emission from the core suggest the presence of a

text: supermassive black hole

text: . Estimates for the mass of this object range from  to  times the mass of the

text: Sun

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answers: NDQ_002618

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answers: galaxy

answers: NDQ_002623

answers: Variations in ultraviolet emission from the core

answers: NDQ_002624

answers: complex galaxy

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: The solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: The universe has billions of galaxies

answers: NDQ_002628

answers: star cluster

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: small inner bulge through the core along with an outer bulge

answers: NDQ_002631

answers: spiral galaxies

answers: NDQ_002632

answers: It is categorized as a double-barred spiral galaxy

answers: NDQ_002633

answers: estimates for the mass of this object range from to times the mass of the Sun

answers: NDQ_002634

answers: The Sun

answers: NDQ_002635

answers: The Sun

answers: NDQ_002636

answers: double-barred spiral galaxy

text: The size and shape of any device is largely driven by the size and shape of the components used to make that device. Traditional HDDs and optical drives are designed around the rotating platter(s) or optical disc along with the spindle motor inside. If an SSD is made up of various interconnected integrated circuits (ICs) and an interface connector, then its shape is no longer limited to the shape of rotating media drives. Some solid state storage solutions come in a larger chassis that may even be a rack-mount form factor with numerous SSDs inside. They would all connect to a common bus inside the chassis and connect outside the box with a single connector.

text: The size and shape of any device is largely driven by the size and shape of the components used to make that device. Traditional HDDs and

text: optical drives

text: are designed around the rotating

text: platter

text: (s) or

text: optical disc

text: along with the

text: spindle motor

text: inside. If an SSD is made up of various interconnected

text: integrated circuit

text: s (ICs) and an interface connector, then its shape is no longer limited to the shape of rotating media drives. Some solid state storage solutions come in a larger chassis that may even be a rack-mount form factor with numerous SSDs inside. They would all connect to a common bus inside the chassis and connect outside the box with a single connector.

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answers: NDQ_002598

answers: galaxy

answers: NDQ_002599

answers: galaxy

answers: NDQ_002600

answers: stars

answers: NDQ_002601

answers: shape is no longer limited to the shape of rotating media drives

answers: NDQ_002602

answers: galaxies

answers: NDQ_002603

answers: solid state storage solutions

answers: NDQ_002604

answers: spinning platter(s)

answers: NDQ_002605

answers: stars

answers: NDQ_002606

answers: ICs

answers: NDQ_002607

answers: are made up of various interconnected integrated circuits

answers: NDQ_002609

answers: billions of stars

answers: NDQ_002610

answers: galaxy

answers: NDQ_002612

answers: platter(s)

answers: NDQ_002615

answers: HDDs

answers: NDQ_002617

answers: galaxy

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: HDD

answers: NDQ_002620

answers: The size and shape of any device is largely driven by the size and shape of the components used to make that device

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: unanswerable

answers: NDQ_002623

answers: The size and shape of any device

answers: NDQ_002624

answers: galaxies

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: rotating platter(s) or optical disc

answers: NDQ_002627

answers: galaxies

answers: NDQ_002628

answers: Star clusters

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: The size and shape

answers: NDQ_002631

answers: Spiral galaxies

answers: NDQ_002632

answers: dwarf galaxies are often found near larger galaxies

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: galaxy

answers: NDQ_002635

answers: Our solar system orbits the central disk of our galaxy

answers: NDQ_002636

answers: galaxy

text: DDO 190 is small, but not tiny: about 15,000 light years across—about 1/6 the size of our galaxy. It is also well outside the Local Group, which contains nearby galaxies (the Andromeda galaxy is less than 3 million light years distant from Earth, for comparison), and is instead thought to be part of the M94 galaxy group. But if true it is fairly isolated even from the others on its team; the nearest neighbor appears to be another dwarf galaxy, DDO 187, at a distance of .

text: DDO 190 is small, but not tiny: about 15,000 light years across—about 1/6 the size of our galaxy. It is also well outside the

text: Local Group

text: , which contains nearby galaxies (the Andromeda galaxy is less than 3 million light years distant from Earth, for comparison), and is instead thought to be part of the

text: M94 galaxy group

text: . But if true it is fairly isolated even from the others on its team; the nearest neighbor appears to be another dwarf galaxy,

text: DDO 187

text: , at a distance of .

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answers: 1/6 the size

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answers: dwarf galaxy

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answers: dwarf galaxy

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answers: dwarf galaxy

answers: NDQ_002617

answers: dwarf galaxy

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: dwarf galaxy

answers: NDQ_002620

answers: dwarf galaxy

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: dwarf galaxy

answers: NDQ_002623

answers: dwarf galaxy

answers: NDQ_002624

answers: dwarf galaxy

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Earth

answers: NDQ_002627

answers: galaxy group

answers: NDQ_002628

answers: galaxy group

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: dwarf

answers: NDQ_002631

answers: DDO 190

answers: NDQ_002632

answers: DDO 187

answers: NDQ_002633

answers: dwarf galaxy

answers: NDQ_002634

answers: Earth

answers: NDQ_002635

answers: Earth orbits the central disk of our galaxy.

answers: NDQ_002636

answers: DDO 190

text: The dynamics of these objects, if they do exist, must be quite different from that of standard star clusters. With a very narrow mass range (all brown dwarfs or white dwarfs), the evaporation rate of these RAMBOs should be very slow as predicted by the evolution of simulated mono-component cluster models. Theoretically, these very long-lived objects could exist in large numbers. The presence of a clustered thick disk-like component of dark matter in the Galaxy has been suggested by Sanchez-Salcedo (1997, 1999) and Kerins (1997).

text: The dynamics of these objects, if they do exist, must be quite different from that of standard star clusters. With a very narrow mass range (all brown dwarfs or white dwarfs), the evaporation rate of these RAMBOs should be very slow as predicted by the evolution of simulated mono-component cluster models. Theoretically, these very long-lived objects could exist in large numbers. The presence of a clustered thick disk-like component of

text: dark matter

text: in the

text: Galaxy

text: has been suggested by Sanchez-Salcedo (1997, 1999) and Kerins (1997).

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answers: NDQ_002598

answers: brown dwarfs or white dwarfs

answers: NDQ_002599

answers: large numbers

answers: NDQ_002600

answers: dark matter

answers: NDQ_002601

answers: with a very narrow mass range

answers: NDQ_002602

answers: white dwarfs

answers: NDQ_002603

answers: elliptical galaxy

answers: NDQ_002604

answers: very narrow mass range

answers: NDQ_002605

answers: brown dwarfs or white dwarfs

answers: NDQ_002606

answers: RAMBOs

answers: NDQ_002607

answers: a clustered thick disk-like component of dark matter

answers: NDQ_002609

answers: dark matter

answers: NDQ_002610

answers: dark matter

answers: NDQ_002612

answers: RAMBOs

answers: NDQ_002615

answers: RAMBOs

answers: NDQ_002617

answers: RAMBOs

answers: NDQ_002618

answers: star clusters

answers: NDQ_002619

answers: RAMBOs

answers: NDQ_002620

answers: brown dwarfs or white dwarfs

answers: NDQ_002621

answers: RAMBOs

answers: NDQ_002622

answers: RAMBOs

answers: NDQ_002623

answers: Brown dwarfs or white dwarfs

answers: NDQ_002624

answers: RAMBOs

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: It has been suggested by Sanchez-Salcedo

answers: NDQ_002627

answers: It has been suggested by Sanchez-Salcedo

answers: NDQ_002628

answers: Galaxies

answers: NDQ_002629

answers: open star clusters

answers: NDQ_002630

answers: white dwarfs

answers: NDQ_002631

answers: Theoretically, these very long-lived objects could exist in large numbers

answers: NDQ_002632

answers: Dwarf galaxies are often found near larger galaxies

answers: NDQ_002633

answers: RAMBOs

answers: NDQ_002634

answers: galaxy

answers: NDQ_002635

answers: Dark matter

answers: NDQ_002636

answers: Galaxy

text: Day shapes are black in color and their sizes are determined by the ColRegs, for instance the size of the ball is not less than 0.6 meter diameter.  The vertical distance between shapes is at least 1.5 meters.  Vessels of less than 20 meters length may use shapes of smaller size commensurate with the size of the vessel. Day shapes of standard and reduced sizes are both commercially available. Day shapes are commonly constructed from a light weight frame covered with fabric and are designed to be collapsible for ease of storage.

text: Day shapes are black in color and their sizes are determined by the ColRegs, for instance the size of the ball is not less than 0.6 meter diameter.  The vertical distance between shapes is at least 1.5 meters.  Vessels of less than 20 meters length may use shapes of smaller size commensurate with the size of the vessel. Day shapes of standard and reduced sizes are both commercially available. Day shapes are commonly constructed from a light weight frame covered with fabric and are designed to be collapsible for ease of storage.

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answers: NDQ_002598

answers: Day shapes

answers: NDQ_002599

answers: billions

answers: NDQ_002600

answers: Day shapes

answers: NDQ_002601

answers: their sizes are determined by the ColRegs

answers: NDQ_002602

answers: galaxies

answers: NDQ_002603

answers: collapsible for ease of storage

answers: NDQ_002604

answers: Day shapes

answers: NDQ_002605

answers: galaxies

answers: NDQ_002606

answers: Day shapes

answers: NDQ_002607

answers: are black in color

answers: NDQ_002609

answers: billions of stars

answers: NDQ_002610

answers: Day shapes

answers: NDQ_002612

answers: Day shapes

answers: NDQ_002615

answers: Day shapes

answers: NDQ_002617

answers: Day shapes

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: Day shapes

answers: NDQ_002620

answers: Day shapes of standard and reduced sizes are both commercially available

answers: NDQ_002621

answers: ColRegs

answers: NDQ_002622

answers: Day shapes

answers: NDQ_002623

answers: It's impossible to say

answers: NDQ_002624

answers: Day shapes

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is rotating around our galaxy.

answers: NDQ_002627

answers: galaxies

answers: NDQ_002628

answers: Star clusters

answers: NDQ_002629

answers: globular star clusters

answers: NDQ_002630

answers: Day shapes

answers: NDQ_002631

answers: It's impossible to say

answers: NDQ_002632

answers: The vertical distance between shapes

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: The vertical distance between shapes is at least 1.5 meters

answers: NDQ_002635

answers: orbits the central disk of our galaxy

answers: NDQ_002636

answers: The vertical distance between shapes

text: DDO 210 (also known as Aquarius Dwarf or PGC 65367) is a dwarf irregular galaxy in the constellation of Aquarius. It is a member of the Local Group and lies 3.2 ± 0.2 million light years from our Milky Way.

text: DDO 210

text: (also known as

text: Aquarius

text: Dwarf

text: or

text: PGC

text: 65367) is a

text: dwarf irregular

text: galaxy

text: in the

text: constellation

text: of

text: Aquarius

text: . It is a member of the

text: Local Group

text: and lies 3.2

text: million

text: light years

text: from our

text: Milky Way

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answers: 2: The answer has limited relevance and completeness, with noticeable gaps or inaccuracies.

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answers: 5

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answers: 4

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answers: 0

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answers: 0

answers: NDQ_002636

answers: 0

answers: NDQ_002598

answers: irregular galaxy

answers: NDQ_002599

answers: Milky Way

answers: NDQ_002600

answers: galaxy

answers: NDQ_002601

answers: constellation

answers: NDQ_002602

answers: dwarf irregular galaxy

answers: NDQ_002603

answers: irregular

answers: NDQ_002604

answers: irregular

answers: NDQ_002605

answers: galaxy

answers: NDQ_002606

answers: irregular

answers: NDQ_002607

answers: dwarf irregular galaxy

answers: NDQ_002609

answers: million light years

answers: NDQ_002610

answers: Milky Way

answers: NDQ_002612

answers: Milky Way

answers: NDQ_002615

answers: dwarf irregular galaxy

answers: NDQ_002617

answers: Milky Way

answers: NDQ_002618

answers: Milky Way

answers: NDQ_002619

answers: Local Group

answers: NDQ_002620

answers: Milky Way

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: dwarf irregular galaxy

answers: NDQ_002623

answers: DDO 210

answers: NDQ_002624

answers: irregular

answers: NDQ_002625

answers: Milky Way

answers: NDQ_002626

answers: Milky Way

answers: NDQ_002627

answers: Milky Way

answers: NDQ_002628

answers: Local Group

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: dwarf irregular

answers: NDQ_002631

answers: irregular

answers: NDQ_002632

answers: Milky Way

answers: NDQ_002633

answers: DDO 210

answers: NDQ_002634

answers: Milky Way

answers: NDQ_002635

answers: Milky Way

answers: NDQ_002636

answers: Milky Way

text: The Corona Borealis Supercluster is a supercluster located in the constellation Corona Borealis and the most prominent example of its kind in the Northern Celestial Hemisphere. Dense and compact compared with other superclusters, its mass has been calculated to lie somewhere between 0.6 and 12 × 10 solar masses (M⊙). It contains the galaxy clusters Abell 2056, Abell 2061, Abell 2065 (the most massive galaxy cluster within the supercluster), Abell 2067, Abell 2079, Abell 2089, and Abell 2092. Of these, Abell 2056, 2061, 2065, 2067 and A2089 are gravitationally bound and in the process of collapsing to form a massive cluster. This entity has an estimated mass of around 1 × 10 M⊙.  If there is inter-cluster mass present, then Abell 2092 may also be involved. It has been estimated to be 100 megaparsecs (330 million light-years) wide and 40 megaparsecs  (130 million light years)  deep. It has a redshift of 0.07, which is equivalent to a distance of around 265.5 megaparsecs (964 million light-years).

text: The Corona Borealis Supercluster is a

text: supercluster

text: located in the constellation

text: Corona Borealis

text: and the most prominent example of its kind in the

text: Northern Celestial Hemisphere

text: . Dense and compact compared with other superclusters, its mass has been calculated to lie somewhere between 0.6 and 12 × 10

text: solar mass

text: es (M⊙). It contains the galaxy clusters

text: Abell 2056

text: Abell 2061

text: Abell 2065

text: (the most massive galaxy cluster within the supercluster),

text: Abell 2067

text: Abell 2079

text: Abell 2089

text: , and

text: Abell 2092

text: . Of these, Abell 2056, 2061, 2065, 2067 and A2089 are gravitationally bound and in the process of collapsing to form a massive cluster. This entity has an estimated mass of around 1 × 10 M⊙.  If there is inter-cluster mass present, then Abell 2092 may also be involved. It has been estimated to be 100

text: megaparsecs

text: (330 million

text: light-year

text: s) wide and 40 megaparsecs  (130 million light years)  deep. It has a redshift of 0.07, which is equivalent to a distance of around 265.5 megaparsecs (964 million light-years).

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answers: 3: The answer has limited relevance and completeness, with noticeable gaps or inaccuracy.

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answers: galaxy clusters

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answers: 12  10 solar masses

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answers: galaxy clusters

answers: NDQ_002601

answers: redshift

answers: NDQ_002602

answers: galaxy clusters

answers: NDQ_002603

answers: compact

answers: NDQ_002604

answers: dense and compact

answers: NDQ_002605

answers: galaxy clusters

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answers: galaxy clusters

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answers: supercluster

answers: NDQ_002609

answers: 12  10 solar masses

answers: NDQ_002610

answers: supercluster

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answers: galaxy cluster

answers: NDQ_002615

answers: supercluster

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answers: supercluster

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answers: The Milky Way

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answers: supercluster

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answers: superclusters

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answers: supercluster

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answers: supercluster

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answers: The Corona Borealis Supercluster

answers: NDQ_002624

answers: supercluster

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: The Corona Borealis Supercluster

answers: NDQ_002627

answers: It has been estimated to be 100 megaparsecs (330 million light-years) wide and 40 megaparsecs (130 million light years) deep

answers: NDQ_002628

answers: galaxy clusters

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: supercluster

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answers: The Corona Borealis Supercluster

answers: NDQ_002632

answers: It contains the galaxy clusters Abell 2056, 2061, 2065

answers: NDQ_002633

answers: The Corona Borealis Supercluster

answers: NDQ_002634

answers: Corona Borealis

answers: NDQ_002635

answers: Our solar system orbits the central disk of our galaxy.

answers: NDQ_002636

answers: Corona Borealis

text: The Milky Way was once considered an ordinary spiral galaxy. Astronomers first began to suspect that the Milky Way is a barred spiral galaxy in the 1990s. Their suspicions were confirmed by Spitzer Space Telescope observations in 2005, which showed that the Milky Way's central bar is larger than was previously suspected.

text: The

text: Milky Way

text: was once considered an ordinary spiral galaxy. Astronomers first began to suspect that the Milky Way is a barred spiral galaxy in the 1990s. Their suspicions were confirmed by

text: Spitzer Space Telescope

text: observations in 2005, which showed that the Milky Way's central bar is larger than was previously suspected.

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answers: NDQ_002598

answers: ordinary spiral galaxy

answers: NDQ_002599

answers: galaxy

answers: NDQ_002600

answers: bar

answers: NDQ_002601

answers: barred

answers: NDQ_002602

answers: ordinary spiral galaxy

answers: NDQ_002603

answers: elliptical

answers: NDQ_002604

answers: bar

answers: NDQ_002605

answers: galaxy

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answers: barred

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answers: The Milky Way

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answers: billions of stars

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answers: bar

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answers: spiral galaxy

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answers: galaxy

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answers: The Milky Way

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: galaxy

answers: NDQ_002620

answers: ordinary spiral galaxy

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxy

answers: NDQ_002623

answers: The Milky Way

answers: NDQ_002624

answers: barred

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: The Milky Way

answers: NDQ_002628

answers: Star clusters

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answers: Open star clusters

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answers: barred spiral

answers: NDQ_002631

answers: It was once considered an ordinary spiral galaxy

answers: NDQ_002632

answers: The Milky Way

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answers: Galaxy

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answers: The Milky Way

answers: NDQ_002635

answers: The Milky Way

answers: NDQ_002636

answers: The Milky Way

text: Some examples are Messier 49 (elliptical), Messier 58 (spiral), Messier 59 (elliptical), Messier 60 (elliptical), Messier 61 (spiral), Messier 84 (lenticular), Messier 86 (lenticular), Messier 87 (elliptical and a famous radio source), Messier 89 (elliptical) and Messier 90 (spiral). A noted galaxy that is not part of the cluster is the Sombrero Galaxy (M104), an unusual spiral galaxy. It is located about 10° due west of Spica.

text: Some examples are

text: Messier 49

text: elliptical

text: Messier 58

text: spiral

text: Messier 59

text: (elliptical),

text: Messier 60

text: (elliptical),

text: Messier 61

text: (spiral),

text: Messier 84

text: lenticular

text: Messier 86

text: (lenticular),

text: Messier 87

text: (elliptical and a famous

text: radio source

text: Messier 89

text: (elliptical) and

text: Messier 90

text: (spiral). A noted galaxy that is not part of the cluster is the

text: Sombrero Galaxy

text: (M104), an unusual spiral galaxy. It is located about 10° due west of Spica.

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answers: 2: The answer has limited relevance and completeness, with significant gaps or inaccuracy.

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text: NGC 176 is an open cluster located around 3.5 million light-years in the constellation Tucana. This cluster consists of several stars together with another galaxy making it one of the most fascinating galaxies among nearby galaxies. It was discovered on August 12, 1834 by John Herschel.

text: NGC

text: 176 is an open cluster located around 3.5 million light-years in the constellation

text: Tucana

text: . This cluster consists of several stars together with another galaxy making it one of the most fascinating galaxies among nearby galaxies. It was discovered on August 12, 1834 by

text: John Herschel

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text: The current model for the universe, ɅCDM, indicates that galaxies tend to cluster and achieve a web-like structure over time. Under such models, the large majority of baryons entering a galactic halo do so along these cosmic filaments. 70% of the mass inflow at the virial radius is consistent with coming in along cosmic filaments in evolutionary models of the Milky Way. Given current observational limitations, the majority of the filaments feeding into the Milky Way are not visible in HI. Despite this, some gas clouds within the Galaxy's halo have lower metallicities than that of gas stripped from satellites, suggesting that the clouds are primordial material probably flowing in along the cosmic filaments. Gas of this type, detectable out to ~160,000 ly (50 kpc), largely becomes part of the hot halo, cools and condenses, and falls into the Galactic disk to serve in star formation.

text: The current model for the universe, ɅCDM, indicates that galaxies tend to cluster and achieve a web-like structure over time. Under such models, the large majority of baryons entering a galactic halo do so along these cosmic filaments. 70% of the mass inflow at the

entity_section: Galaxies and cosmology .28virial mass and radius.29

text: virial radius

text: is consistent with coming in along cosmic filaments in evolutionary models of the Milky Way. Given current observational limitations, the majority of the filaments feeding into the Milky Way are not visible in HI. Despite this, some gas clouds within the Galaxy's halo have lower metallicities than that of gas stripped from satellites, suggesting that the clouds are primordial material probably flowing in along the cosmic filaments. Gas of this type, detectable out to ~160,000 ly (50 kpc), largely becomes part of the hot halo, cools and condenses, and falls into the Galactic disk to serve in star formation.

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answers: NDQ_002599

answers: Galactic disk

answers: NDQ_002600

answers: cosmic filaments

answers: NDQ_002601

answers: web-like structure

answers: NDQ_002602

answers: Milky Way

answers: NDQ_002603

answers: galaxy tend to cluster and achieve a web-like structure

answers: NDQ_002604

answers: cosmic filaments

answers: NDQ_002605

answers: Galactic disk

answers: NDQ_002606

answers: galaxy

answers: NDQ_002607

answers: galaxy's halo

answers: NDQ_002609

answers: 160,000 ly

answers: NDQ_002610

answers: cosmic filaments

answers: NDQ_002612

answers: Milky Way

answers: NDQ_002615

answers: Milky Way

answers: NDQ_002617

answers: Milky Way

answers: NDQ_002618

answers: HI

answers: NDQ_002619

answers: halo

answers: NDQ_002620

answers: Milky Way

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxies

answers: NDQ_002623

answers: galaxy's halo

answers: NDQ_002624

answers: Milky Way

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: The Milky Way

answers: NDQ_002627

answers: The current model for the universe

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: Milky Way

answers: NDQ_002631

answers: spiral galaxies

answers: NDQ_002632

answers: The Milky Way

answers: NDQ_002633

answers: The Milky Way

answers: NDQ_002634

answers: The Milky Way

answers: NDQ_002635

answers: Galactic disk

answers: NDQ_002636

answers: web-like structure

text: This spiral galaxy is notably asymmetric.  The spiral arms on the south side of the galaxy are chaotic in appearance, whereas the spiral arms on the north side of the galaxy are very well-defined.  Also, the spiral arms on the south side of the disk extend twice as far from the galaxy's nucleus as the spiral arms on the north side.  Because of the fragmentary appearance of some of the spiral arms, this galaxy is classified as a flocculent galaxy.

text: This spiral galaxy is notably asymmetric.  The

text: spiral arm

text: s on the south side of the galaxy are chaotic in appearance, whereas the spiral arms on the north side of the galaxy are very well-defined.  Also, the spiral arms on the south side of the disk extend twice as far from the galaxy's

text: nucleus

text: as the spiral arms on the north side.  Because of the fragmentary appearance of some of the spiral arms, this galaxy is classified as a

text: flocculent galaxy

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answers: NDQ_002602

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answers: NDQ_002603

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answers: NDQ_002604

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answers: NDQ_002605

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text: For a filter to be compatible with a coffee maker, the filter needs to be a specific shape and size.  Common in the US are cone-shaped filters #2, #4, and #6, as well as basket-shaped filters in an 8-12 cup size.

text: For a filter to be compatible with a coffee maker, the filter needs to be a specific shape and size.  Common in the US are cone-shaped filters #2, #4, and #6, as well as basket-shaped filters in an 8-12 cup size.

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answers: NDQ_002610

answers: coffee maker

answers: NDQ_002612

answers: cone

answers: NDQ_002615

answers: 8-12 cup

answers: NDQ_002617

answers: basket-shaped

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: galaxy

answers: NDQ_002620

answers: cone-shaped filters

answers: NDQ_002621

answers: stars

answers: NDQ_002622

answers: 8-12 cup

answers: NDQ_002623

answers: basket-shaped filters

answers: NDQ_002624

answers: basket-shaped

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system revolves around our galaxy.

answers: NDQ_002627

answers: galaxies

answers: NDQ_002628

answers: Star clusters

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: basket-shaped

answers: NDQ_002631

answers: Spiral

answers: NDQ_002632

answers: Dwarf galaxies

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: The solar system is located within the Milky Way galaxy.

answers: NDQ_002635

answers: orbits the central disk of our galaxy

answers: NDQ_002636

answers: cone-shaped

text: The number density of galaxies in the LS falls off with the square of the distance from its center near the Virgo Cluster, suggesting that this cluster is not randomly located. Overall, the vast majority of the luminous galaxies (less than absolute magnitude −13) are concentrated in a small number of clouds (groups of galaxy clusters). Ninety-eight percent can be found in the following 11 clouds (given in decreasing order of number of luminous galaxies): Canes Venatici, Virgo Cluster, Virgo II (southern extension), Leo II, Virgo III, Crater (NGC 3672), Leo I, Leo Minor (NGC 2841), Draco (NGC 5907), Antlia (NGC 2997) and NGC 5643. Of the luminous galaxies located in the disk, one third are in the Virgo Cluster, while the remainder are found in the Canes Venatici Cloud and Virgo II Cloud, plus the somewhat insignificant NGC 5643 Group. The luminous galaxies in the halo are also concentrated in a small number of clouds (94% in 7 clouds). This distribution indicates that "most of the volume of the supergalactic plane is a great void." A helpful analogy that matches the observed distribution is that of soap bubbles. Flattish clusters and superclusters are found at the intersection of bubbles, which are large, roughly spherical (on the order of 20–60 Mpc in diameter) voids in space.Long filamentary structures seem to predominate. An example of this is the Hydra-Centaurus Supercluster, the nearest supercluster to the LS, which starts at a distance of roughly 30 Mpc and extends to 60 Mpc.

text: The

text: number density

text: of galaxies in the LS falls off with the square of the distance from its center near the

text: Virgo Cluster

text: , suggesting that this cluster is not randomly located. Overall, the vast majority of the luminous galaxies (less than

text: absolute magnitude

text: −13) are concentrated in a small number of

text: clouds

text: (groups of

text: galaxy cluster

text: s). Ninety-eight percent can be found in the following 11 clouds (given in decreasing order of number of luminous galaxies):

text: Canes Venatici

text: , Virgo Cluster, Virgo II (southern extension), Leo II, Virgo III, Crater (NGC 3672), Leo I, Leo Minor (NGC 2841), Draco (NGC 5907), Antlia (NGC 2997) and NGC 5643. Of the luminous galaxies located in the disk, one third are in the Virgo Cluster, while the remainder are found in the Canes Venatici Cloud and Virgo II Cloud, plus the somewhat insignificant NGC 5643 Group. The luminous galaxies in the halo are also concentrated in a small number of clouds (94% in 7 clouds). This distribution indicates that "most of the volume of the supergalactic plane is a great void." A helpful analogy that matches the observed distribution is that of soap bubbles. Flattish clusters and

text: superclusters

text: are found at the intersection of bubbles, which are large, roughly spherical (on the order of 20–60

text: Mpc

text: in diameter) voids in space.Long filamentary structures seem to predominate. An example of this is the

text: Hydra-Centaurus Supercluster

text: , the nearest supercluster to the LS, which starts at a distance of roughly 30 Mpc and extends to 60 Mpc.

answers: tqa2:L_0062/T_0626/0ca13908895d7adcb5d4f7bf27bc2b3a

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answers: 0: The answer is not relevant or complete at all.

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answers: 0: The answer is not relevant or complete at all.

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answers: 0: The answer is not relevant or complete at all.

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answers: 3: The answer has limited relevance and completeness, with noticeable gaps or inaccuracy.

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answers: 3: The answer has limited relevance and completeness, with noticeable gaps or inaccuracies.

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answers: 1: The answer is not relevant or complete, with substantial shortcomings.

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answers: NDQ_002598

answers: 4

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answers: NDQ_002600

answers: 0

answers: NDQ_002601

answers: 0

answers: NDQ_002602

answers: 4

answers: NDQ_002603

answers: 0

answers: NDQ_002604

answers: 0

answers: NDQ_002605

answers: 0

answers: NDQ_002606

answers: 0

answers: NDQ_002607

answers: 4

answers: NDQ_002609

answers: 0

answers: NDQ_002610

answers: 0

answers: NDQ_002612

answers: 0

answers: NDQ_002615

answers: 0

answers: NDQ_002617

answers: 0

answers: NDQ_002618

answers: 0

answers: NDQ_002619

answers: 0

answers: NDQ_002620

answers: 0

answers: NDQ_002621

answers: 0

answers: NDQ_002622

answers: 0

answers: NDQ_002623

answers: 0

answers: NDQ_002624

answers: 0

answers: NDQ_002625

answers: 0

answers: NDQ_002626

answers: 0

answers: NDQ_002627

answers: 4

answers: NDQ_002628

answers: 4

answers: NDQ_002629

answers: 3

answers: NDQ_002630

answers: 0

answers: NDQ_002631

answers: 0

answers: NDQ_002632

answers: 2

answers: NDQ_002633

answers: 0

answers: NDQ_002634

answers: 0

answers: NDQ_002635

answers: 0

answers: NDQ_002636

answers: 0

answers: NDQ_002598

answers: Virgo Cluster

answers: NDQ_002599

answers: less than absolute magnitude  13

answers: NDQ_002600

answers: galaxies

answers: NDQ_002601

answers: Long filamentary structures seem to predominate

answers: NDQ_002602

answers: galaxy clusters

answers: NDQ_002603

answers: most of the volume of the supergalactic plane is a great void

answers: NDQ_002604

answers: voids in space

answers: NDQ_002605

answers: long filamentary structures

answers: NDQ_002606

answers: Flattish

answers: NDQ_002607

answers: are large, roughly spherical

answers: NDQ_002609

answers: 60 Mpc

answers: NDQ_002610

answers: Virgo Cluster

answers: NDQ_002612

answers: disk

answers: NDQ_002615

answers: galaxy clusters

answers: NDQ_002617

answers: Virgo Cluster

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: cloud

answers: NDQ_002620

answers: Ninety-eight percent can be found in the 11 clouds

answers: NDQ_002621

answers: galaxy cluster

answers: NDQ_002622

answers: Virgo Cluster

answers: NDQ_002623

answers: Long filamentary structures seem to predominate

answers: NDQ_002624

answers: halo

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: It is not randomly located.

answers: NDQ_002627

answers: Galaxy clusters

answers: NDQ_002628

answers: Galaxy clusters

answers: NDQ_002629

answers: globular star clusters

answers: NDQ_002630

answers: Long filamentary structures

answers: NDQ_002631

answers: Spiral galaxies

answers: NDQ_002632

answers: Canes Venatici Cloud and Virgo II Cloud

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: halo

answers: NDQ_002635

answers: The halo

answers: NDQ_002636

answers: Virgo Cluster

text: The Large Magellanic Cloud (LMC) is a satellite galaxy of the Milky Way. At a distance of 50 kiloparsecs (≈163,000 light-years), the LMC is the third-closest galaxy to the Milky Way, after the Sagittarius Dwarf Spheroidal (~ 16 kpc) and the putative Canis Major Dwarf Galaxy (~ 12.9 kpc, though its status as a galaxy is under dispute) lying closer to the center of the Milky Way. The LMC has a diameter of about  and a mass of approximately 10 billion Sun masses (10 solar masses), making it roughly 1/100 as massive as the Milky Way. The LMC is the fourth-largest galaxy in the Local Group, after the Andromeda Galaxy (M31), the Milky Way, and the Triangulum Galaxy (M33).

text: The Large Magellanic Cloud (LMC) is a

text: satellite galaxy

text: of the

text: Milky Way

text: . At a distance of 50

text: kiloparsecs

text: light-year

text: s), the LMC is the third-closest galaxy to the Milky Way, after the

text: Sagittarius Dwarf Spheroidal

text: (~ 16 kpc) and the

text: putative

text: Canis Major Dwarf Galaxy

text: (~ 12.9 kpc, though its status as a galaxy is under

text: dispute

text: ) lying closer to the center of the Milky Way. The LMC has a diameter of about  and a mass of approximately 10 billion Sun masses (10

text: solar mass

text: es), making it roughly 1/100 as massive as the Milky Way. The LMC is the fourth-largest galaxy in the

text: Local Group

text: , after the

text: Andromeda Galaxy

text: (M31), the Milky Way, and the

text: Triangulum Galaxy

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text: The Canis Major Dwarf Galaxy (CMa Dwarf) or Canis Major Overdensity (CMa Overdensity) is a disputed dwarf irregular galaxy in the Local Group, located in the same part of the sky as the constellation Canis Major.

text: The Canis Major Dwarf Galaxy (CMa Dwarf) or Canis Major Overdensity (CMa Overdensity) is a disputed

text: dwarf irregular galaxy

text: in the

text: Local Group

text: , located in the same part of the sky as the

text: constellation

text: Canis Major

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text: In 1997 and in Heidelberg Kroupa, together with Ulrich Bastian, took the first precise measurement of the spatial movement of two extragalactic systems. In 1997 he also discovered stellar-dynamic solutions for the satellite galaxies of the Milky Way without the need for exotic dark matter. His work implies a possible connection of the satellite galaxies with the Bulge of the Milky Way. This connection can be explained by a collision of the early Milky Way with another young galaxy during which the satellite galaxies formed as tidal dwarf galaxies about 11 Gyr ago. This is shown in a series of research papers with Manuel Metz and Marcel Pawlowski.

text: In 1997 and in Heidelberg Kroupa, together with Ulrich Bastian, took the first precise measurement of the spatial movement of two extragalactic systems. In 1997 he also discovered stellar-dynamic solutions for the

text: satellite galaxies of the Milky Way

text: without the need for exotic

text: dark matter

text: . His work implies a possible connection of the satellite galaxies with the Bulge of the Milky Way. This connection can be explained by a collision of the early Milky Way with another young galaxy during which the satellite galaxies formed as

text: tidal dwarf galaxies

text: about 11 Gyr ago. This is shown in a series of research papers with Manuel Metz and Marcel Pawlowski.

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answers: NDQ_002598

answers: 0

answers: NDQ_002599

answers: 0

answers: NDQ_002600

answers: 0

answers: NDQ_002601

answers: 0

answers: NDQ_002602

answers: 4

answers: NDQ_002603

answers: 0

answers: NDQ_002604

answers: 0

answers: NDQ_002605

answers: 0

answers: NDQ_002606

answers: 0

answers: NDQ_002607

answers: 0

answers: NDQ_002609

answers: 0

answers: NDQ_002610

answers: 4

answers: NDQ_002612

answers: 0

answers: NDQ_002615

answers: 0

answers: NDQ_002617

answers: 0

answers: NDQ_002618

answers: 0

answers: NDQ_002619

answers: 0

answers: NDQ_002620

answers: 4

answers: NDQ_002621

answers: 0

answers: NDQ_002622

answers: 0

answers: NDQ_002623

answers: 0

answers: NDQ_002624

answers: 0

answers: NDQ_002625

answers: 0

answers: NDQ_002626

answers: 4

answers: NDQ_002627

answers: 4

answers: NDQ_002628

answers: 4

answers: NDQ_002629

answers: 3

answers: NDQ_002630

answers: 0

answers: NDQ_002631

answers: 2

answers: NDQ_002632

answers: 4

answers: NDQ_002633

answers: 4

answers: NDQ_002634

answers: 4

answers: NDQ_002635

answers: 4

answers: NDQ_002636

answers: 4

answers: NDQ_002598

answers: dwarf galaxies

answers: NDQ_002599

answers: 11 Gyr

answers: NDQ_002600

answers: dark matter

answers: NDQ_002601

answers: stellar-dynamic solutions

answers: NDQ_002602

answers: Milky Way

answers: NDQ_002603

answers: elliptical

answers: NDQ_002604

answers: galaxies

answers: NDQ_002605

answers: galaxies

answers: NDQ_002606

answers: dwarf galaxies

answers: NDQ_002607

answers: satellite galaxies

answers: NDQ_002609

answers: 11 Gyr

answers: NDQ_002610

answers: Bulge

answers: NDQ_002612

answers: tidal

answers: NDQ_002615

answers: galaxies

answers: NDQ_002617

answers: Milky Way

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: dwarf galaxies

answers: NDQ_002620

answers: Milky Way

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: dwarf galaxies

answers: NDQ_002623

answers: galaxies

answers: NDQ_002624

answers: tidal

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The Milky Way

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: dwarf galaxies

answers: NDQ_002631

answers: spiral

answers: NDQ_002632

answers: satellite galaxies

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: The Milky Way

answers: NDQ_002635

answers: Milky Way

answers: NDQ_002636

answers: Milky Way

text:
Column 1: Name of the galaxy
Column 2: Right ascension for epoch J2000
Column 3: Declination for epoch J2000
Column 4: Blue apparent magnitude of the galaxy
Column 5: Galaxy type: E=Elliptical; S0=Lenticular; Sa, Sb, Sc, Sd=Spiral (degree of woundedness of spiral arms); SBa, SBb, SBc, SBd=Barred Spiral; SAB= Intermediate Spiral (between barred and unbarred); Sm, SBm, Irr=Irregular; (r),(rs)=Ring Structure
Column 6: Angular diameter of the galaxy (arcminutes)
Column 7: Diameter of the galaxy (thousands of light years)
Column 8: Recessional velocity (km/s) of the galaxy relative to the cosmic microwave background

text: Column 1: Name of the

text: galaxy

text: <br>Column 2:

text: Right ascension

text: for

text: epoch J2000

text: <br>Column 3:

text: Declination

text: for epoch J2000<br>Column 4: Blue

text: apparent magnitude

text: of the galaxy<br>Column 5:

text: Galaxy type

text: : E=Elliptical; S0=Lenticular; Sa, Sb, Sc, Sd=Spiral (degree of woundedness of spiral arms); SBa, SBb, SBc, SBd=Barred Spiral; SAB= Intermediate Spiral (between barred and unbarred); Sm, SBm, Irr=Irregular; (r),(rs)=Ring Structure<br>Column 6: Angular diameter of the galaxy (

text: arcminutes

text:
)
Column 7: Diameter of the galaxy (thousands of light years)
Column 8: Recessional velocity (km/s) of the galaxy relative to the

text: cosmic microwave background

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answers: 3: The answer has limited relevance and completeness, with noticeable gaps or inaccuracies.

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answers: 0

answers: NDQ_002598

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answers: NDQ_002604

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answers: NDQ_002605

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answers: 5

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answers: NDQ_002619

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answers: NDQ_002620

answers: 4

answers: NDQ_002621

answers: 0

answers: NDQ_002622

answers: 0

answers: NDQ_002623

answers: 3

answers: NDQ_002624

answers: 3

answers: NDQ_002625

answers: 0

answers: NDQ_002626

answers: 4

answers: NDQ_002627

answers: 0

answers: NDQ_002628

answers: 4

answers: NDQ_002629

answers: 3

answers: NDQ_002630

answers: 4

answers: NDQ_002631

answers: 3

answers: NDQ_002632

answers: 3

answers: NDQ_002633

answers: 0

answers: NDQ_002634

answers: 4

answers: NDQ_002635

answers: 0

answers: NDQ_002636

answers: 4

answers: NDQ_002598

answers: Sm, SBm, Irr, Ring Structure

answers: NDQ_002599

answers: thousands of stars

answers: NDQ_002600

answers: Spirals

answers: NDQ_002601

answers: Ring Structure

answers: NDQ_002602

answers: Galaxy type: E=Elliptical; S0=Lenticular; Sa, Sb, Sc, Sd=Spiral (degree of woundedness of spiral arms); SBa, SBb, SBc, SBd=Barred Spiral; SAB=Intermediate Spiral (between barred and unbarred); Sm, SBm, Irr=Irregular; (r),(rs)=Ring Structure

answers: NDQ_002603

answers: The galaxy is elliptical.

answers: NDQ_002604

answers: Spiral galaxies have a degree of woundedness of spiral arms.

answers: NDQ_002605

answers: The stars in an open cluster are mostly

answers: NDQ_002606

answers: Irregular

answers: NDQ_002607

answers: Galaxy type: E=Elliptical; S0=Lenticular; Sa, Sb, Sc, Sd=Spiral (degree of woundedness of spiral arms); SBa, SBb, SBc, SBd=Barred Spiral; SAB=Intermediate Spiral (between barred and unbarred); Sm, SBm, Irr=Irregular; (r),(rs)=Ring Structure

answers: NDQ_002609

answers: 1 billion stars

answers: NDQ_002610

answers: Spiral

answers: NDQ_002612

answers: spiral galaxy

answers: NDQ_002615

answers: galaxy

answers: NDQ_002617

answers: Elliptical

answers: NDQ_002618

answers: The Milky Way appears as a band of light across the night sky.

answers: NDQ_002619

answers: cosmic microwave background

answers: NDQ_002620

answers: Galaxy type: E=Elliptical; S0=Lenticular; Sa, Sb, Sc, Sd=Spiral (degree of woundedness of spiral arms); SBa, SBb, SBc, SBd=Barred Spiral; SAB=Intermediate Spiral (between barred and unbarred); Sm, SBm, Irr=Irregular; (r),(rs)=Ring Structure

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxy

answers: NDQ_002623

answers: Galaxy type: E = Elliptical

answers: NDQ_002624

answers: Intermediate Spiral

answers: NDQ_002625

answers: The Milky Way Galaxy is a spiral galaxy.

answers: NDQ_002626

answers: The solar system is rotating around our galaxy.

answers: NDQ_002627

answers: There are billions of galaxies in the universe.

answers: NDQ_002628

answers: A star cluster may contain one or more galaxies

answers: NDQ_002629

answers: Open star clusters contain more stars than globular star clusters.

answers: NDQ_002630

answers: Angular diameter of the galaxy (arcminutes) br>Diameter of the galaxy (thousands of light years) br>Recessional velocity (km/s)

answers: NDQ_002631

answers: Spiral galaxies are generally older than elliptical galaxies.

answers: NDQ_002632

answers: Dwarf galaxies are often found near larger galaxies.

answers: NDQ_002633

answers: Galaxy type: E=Elliptical; S0=Lenticular; Sa, Sb, Sc, Sd=Spiral (degree of woundedness of spiral arms); SBa, SBb, SBc, SBd=Barred Spiral; SAB=Intermediate Spiral; Sm, SBm, Irr=Irregular; (r),(rs)=Ring Structure br>Column 6: Angular diameter of the galaxy (arcminutes) br>Column 7: Diameter of the galaxy (thousands of light years) br>Column 8: Recessional velocity (km/s) of the galaxy relative to the cosmic microwave background

answers: NDQ_002634

answers: The solar system is within one of the spiral arms of our galaxy.

answers: NDQ_002635

answers: The solar system orbits the central disk of our galaxy.

answers: NDQ_002636

answers: Galaxy type: E = Elliptical; S0 = Lenticular; Sa, Sb, Sc, Sd = Spiral; SBa, SBb, SBc, SBd = Barred Spiral; SAB = Intermediate Spiral; Sm, SBm, Irr = Irregular; (r), (rs) = Ring Structure

text: An open cluster is a group of up to a few thousand stars that were formed from the same giant molecular cloud and have roughly the same age. More than 1,100 open clusters have been discovered within the Milky Way Galaxy, and many more are thought to exist. They are loosely bound by mutual gravitational attraction and become disrupted by close encounters with other clusters and clouds of gas as they orbit the galactic center. This can result in a migration to the main body of the galaxy and a loss of cluster members through internal close encounters. Open clusters generally survive for a few hundred million years, with the most massive ones surviving for a few billion years. In contrast, the more massive globular clusters of stars exert a stronger gravitational attraction on their members, and can survive for longer. Open clusters have been found only in spiral and irregular galaxies, in which active star formation is occurring.

text: An open cluster is a

text: group

text: of up to a few thousand

text: star

text: s that were formed from the same

text: giant molecular cloud

text: and have roughly the same age. More than 1,100 open clusters have been discovered within the

text: Milky Way Galaxy

text: , and many more are thought to exist. They are loosely bound by mutual

text: gravitational attraction

text: and become disrupted by close encounters with other clusters and clouds of gas as they orbit the galactic center. This can result in a migration to the main body of the galaxy and a loss of cluster members through internal close encounters. Open clusters generally survive for a few hundred million years, with the most massive ones surviving for a few billion years. In contrast, the more massive

text: globular cluster

text: s of stars exert a stronger gravitational attraction on their members, and can survive for longer. Open clusters have been found only in

text: spiral

text: and

text: irregular galaxies

text: , in which active

text: star formation

text: is occurring.

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answers: 0

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answers: 3

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answers: active star formation

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answers: 4

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answers: 4

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answers: 0

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answers: 0

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answers: 4

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answers: 4

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answers: 4

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answers: 0

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answers: 4

answers: NDQ_002605

answers: 4

answers: NDQ_002606

answers: 4

answers: NDQ_002607

answers: 4

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answers: 4

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answers: 4

answers: NDQ_002612

answers: 4

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answers: 5

answers: NDQ_002617

answers: 0

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answers: 0

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answers: 3

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answers: 4

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answers: 5

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answers: 0

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answers: 0

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answers: 0

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 4

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answers: 2

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answers: 4

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answers: 4

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answers: 4

answers: NDQ_002598

answers: open clusters

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answers: few thousand stars

answers: NDQ_002600

answers: open clusters

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answers: close encounters with other clusters and clouds of gas as they orbit the galactic center

answers: NDQ_002602

answers: spiral and irregular

answers: NDQ_002603

answers: active star formation is occurring

answers: NDQ_002604

answers: active star formation

answers: NDQ_002605

answers: formed from the same giant molecular cloud

answers: NDQ_002606

answers: irregular galaxies

answers: NDQ_002607

answers: more massive globular clusters of stars

answers: NDQ_002609

answers: 1,100 open clusters

answers: NDQ_002610

answers: open cluster

answers: NDQ_002612

answers: spiral

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answers: An open cluster

answers: NDQ_002617

answers: irregular

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answers: galaxy

answers: NDQ_002619

answers: open cluster

answers: NDQ_002620

answers: Milky Way Galaxy

answers: NDQ_002621

answers: open cluster

answers: NDQ_002622

answers: An open cluster

answers: NDQ_002623

answers: globular clusters

answers: NDQ_002624

answers: irregular

answers: NDQ_002625

answers: open clusters

answers: NDQ_002626

answers: The Milky Way Galaxy

answers: NDQ_002627

answers: many more are thought to exist

answers: NDQ_002628

answers: galaxy

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answers: Open star clusters

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answers: Massive

answers: NDQ_002631

answers: spiral

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answers: It can result in a migration to the main body of the galaxy

answers: NDQ_002633

answers: The most massive ones surviving for a few billion years

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answers: Milky Way Galaxy

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answers: galactic center

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answers: Milky Way Galaxy

text: Elliptical galaxies (such as IC 1101) are among some of the largest known thus far. Their stars are on orbits that are randomly oriented within the galaxy (i.e. they are not rotating like disk galaxies). A distinguishing feature of elliptical galaxies is that the velocity of the stars does not necessarily contribute to flattening of the galaxy, such as in spiral galaxies. Elliptical galaxies have supermassive black holes at their center, and the mass of these black holes correlates with the galaxy’s mass.

text: Elliptical galaxies (such as

text: IC 1101

text: ) are among some of the largest known thus far. Their stars are on orbits that are randomly oriented within the galaxy (i.e. they are not rotating like disk galaxies). A distinguishing feature of elliptical galaxies is that the velocity of the stars does not necessarily contribute to flattening of the galaxy, such as in spiral galaxies. Elliptical galaxies have

text: supermassive black hole

text: s at their center, and the mass of these black holes correlates with the galaxy’s mass.

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answers: their stars are on orbits that are randomly oriented

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answers: 4

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answers: 0

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answers: 3

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answers: 4

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answers: 4

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answers: 4

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answers: 2

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answers: 4

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answers: 4

answers: NDQ_002598

answers: disk galaxies

answers: NDQ_002599

answers: largest

answers: NDQ_002600

answers: black holes

answers: NDQ_002601

answers: velocity of the stars does not necessarily contribute to flattening

answers: NDQ_002602

answers: Elliptical

answers: NDQ_002603

answers: their stars are on orbits that are randomly oriented

answers: NDQ_002604

answers: flattening

answers: NDQ_002605

answers: randomly oriented within the galaxy

answers: NDQ_002606

answers: Elliptical

answers: NDQ_002607

answers: are not rotating like disk galaxies

answers: NDQ_002609

answers: billions of stars

answers: NDQ_002610

answers: black holes

answers: NDQ_002612

answers: spiral

answers: NDQ_002615

answers: galaxies

answers: NDQ_002617

answers: Elliptical

answers: NDQ_002618

answers: galaxy

answers: NDQ_002619

answers: disk galaxies

answers: NDQ_002620

answers: disk galaxies

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxies

answers: NDQ_002623

answers: It's impossible to say

answers: NDQ_002624

answers: disk

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: orbits that are randomly oriented

answers: NDQ_002627

answers: It's impossible to say

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: open star clusters

answers: NDQ_002630

answers: Elliptical

answers: NDQ_002631

answers: Spiral galaxies

answers: NDQ_002632

answers: dwarf galaxies

answers: NDQ_002633

answers: Elliptical galaxies

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answers: galaxy

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answers: disk galaxies

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answers: disk galaxies

text: Maffei 1 is a giant elliptical galaxy classified as type E3 in the Hubble classification scheme. This means that it is slightly flattened, its semi-minor axis being 70% of its semi-major axis. Maffei 1 has also a boxy shape (E(b)3 type), while its central region (radius ≈ 34 pc) is deficient in light emission as compared to the r law, meaning that Maffei 1 is a core type elliptical. Both the boxy shape and the presence of an underluminous core are typical of intermediate to massive ellipticals.

text: Maffei 1 is a giant elliptical galaxy classified as type E3 in the

text: Hubble classification

text: scheme. This means that it is slightly flattened, its

text: semi-minor axis

text: being 70% of its

text: semi-major axis

text: . Maffei 1 has also a boxy shape (E(b)3 type), while its central region (radius ≈ 34 pc) is deficient in light emission as compared to the r law, meaning that Maffei 1 is a core type elliptical. Both the boxy shape and the presence of an underluminous core are typical of intermediate to massive ellipticals.

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answers: elliptical

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answers: massive

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answers: an underluminous core

answers: NDQ_002601

answers: boxy shape

answers: NDQ_002602

answers: elliptical

answers: NDQ_002603

answers: an underluminous core

answers: NDQ_002604

answers: boxy shape

answers: NDQ_002605

answers: stars

answers: NDQ_002606

answers: flattened

answers: NDQ_002607

answers: Maffei 1

answers: NDQ_002609

answers: 34 pc

answers: NDQ_002610

answers: core

answers: NDQ_002612

answers: Elliptical

answers: NDQ_002615

answers: Maffei 1

answers: NDQ_002617

answers: elliptical

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: semi-minor

answers: NDQ_002620

answers: giant elliptical galaxy

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: Maffei 1

answers: NDQ_002623

answers: The presence of an underluminous core are typical of intermediate to massive ellipticals

answers: NDQ_002624

answers: type E3

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Maffei 1 is a giant elliptical galaxy

answers: NDQ_002627

answers: The universe has billions of galaxies

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answers: Star cluster

answers: NDQ_002629

answers: Open star clusters

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answers: giant

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answers: elliptical

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answers: Maffei 1

answers: NDQ_002633

answers: Maffei 1

answers: NDQ_002634

answers: Maffei 1 is a giant elliptical galaxy

answers: NDQ_002635

answers: Maffei 1

answers: NDQ_002636

answers: elliptical

text: Some galaxies are irregular and do not have any well-defined disk. Even in the case of a barred spiral galaxy like the Milky Way, defining the galactic plane is slightly imprecise and arbitrary since the stars are not perfectly coplanar. In 1959 the IAU defined the position of the Milky Way's north galactic pole as exactly RA = , Dec =  in the then-used B1950 epoch; in the currently-used J2000 epoch, after precession is taken into account, its position is RA , Dec . This position is in Coma Berenices, near the bright star Arcturus; likewise, the south galactic pole lies in the constellation Sculptor.

text: Some galaxies are irregular and do not have any well-defined disk. Even in the case of a

text: barred spiral galaxy

text: like the Milky Way, defining the galactic plane is slightly imprecise and arbitrary since the stars are not perfectly coplanar. In 1959 the

text: IAU

text: defined the position of the Milky Way's north galactic pole as exactly

text: RA

text: Dec

text: =  in the then-used

text: epoch

text: ; in the currently-used

text: epoch, after

text: precession

text: is taken into account, its position is RA , Dec . This position is in

text: Coma Berenices

text: , near the bright

text: star

text: Arcturus

text: ; likewise, the south galactic pole lies in the

text: constellation

text: Sculptor

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answers: NDQ_002598

answers: galaxy

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answers: galaxy

answers: NDQ_002600

answers: stars

answers: NDQ_002601

answers: stars are not perfectly coplanar

answers: NDQ_002602

answers: barred spiral galaxy

answers: NDQ_002603

answers: stars are not perfectly coplanar

answers: NDQ_002604

answers: stars

answers: NDQ_002605

answers: not perfectly coplanar

answers: NDQ_002606

answers: irregular

answers: NDQ_002607

answers: Coma Berenices

answers: NDQ_002609

answers: stars

answers: NDQ_002610

answers: well-defined disk

answers: NDQ_002612

answers: spiral

answers: NDQ_002615

answers: galaxy

answers: NDQ_002617

answers: barred spiral galaxy

answers: NDQ_002618

answers: bright star Arcturus

answers: NDQ_002619

answers: constellation

answers: NDQ_002620

answers: Milky Way

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: galaxy

answers: NDQ_002623

answers: The Milky Way

answers: NDQ_002624

answers: irregular

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answers: The Milky Way Galaxy

answers: NDQ_002626

answers: precession is taken into account

answers: NDQ_002627

answers: galaxy like the Milky Way

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: spiral galaxy

answers: NDQ_002631

answers: The Milky Way

answers: NDQ_002632

answers: The Milky Way

answers: NDQ_002633

answers: The Milky Way

answers: NDQ_002634

answers: The Milky Way

answers: NDQ_002635

answers: The Milky Way's north galactic pole

answers: NDQ_002636

answers: The Milky Way

text: NGC 772 is a spiral galaxy with an integrated magnitude of 10.3, located southeast of β Arietis and 15 arcminutes west of 15 Arietis. It is a relatively bright galaxy and shows obvious nebulosity and ellipticity in an amateur telescope. It is 7.2 by 4.2 arcminutes, meaning that its surface brightness, magnitude 13.6, is significantly lower than its integrated magnitude. NGC 772 is a class SA(s)b galaxy, which means that it is an unbarred spiral galaxy without a ring that possesses a somewhat prominent bulge and spiral arms that are wound somewhat tightly. The main arm, on the northwest side of the galaxy, is home to many star forming regions; this is due to previous gravitational interactions with other galaxies. NGC 772 has a small companion galaxy, NGC 770, that is about 113,000 light-years away from the larger galaxy. The two galaxies together are also classified as Arp 78 in the Arp peculiar galaxy catalog. NGC 772 has a diameter of 240,000 light-years and the system is 114 million light-years from Earth. Another spiral galaxy in Aries is NGC 673, a face-on class SAB(s)c galaxy. It is a weakly barred spiral galaxy with loosely wound arms. It has no ring and a faint bulge and is 2.5 by 1.9 arcminutes. It has two primary arms with fragments located farther from the core. 171,000 light-years in diameter, NGC 673 is 235 million light-years from Earth.

text: NGC 772

text: is a

text: spiral galaxy

text: with an

text: integrated magnitude

text: of 10.3, located southeast of β Arietis and 15 arcminutes west of

text: 15 Arietis

text: . It is a relatively bright galaxy and shows obvious nebulosity and ellipticity in an amateur telescope. It is 7.2 by 4.2 arcminutes, meaning that its

text: surface brightness

text: , magnitude 13.6, is significantly lower than its integrated magnitude. NGC 772 is a

text: class SA(s)b galaxy

text: , which means that it is an unbarred spiral galaxy without a ring that possesses a somewhat prominent

text: bulge

text: and spiral arms that are wound somewhat tightly. The main arm, on the northwest side of the galaxy, is home to many

text: star forming regions

text: ; this is due to previous

text: gravitational interactions

text: with other galaxies. NGC 772 has a small companion galaxy,

text: NGC 770

text: , that is about 113,000 light-years away from the larger galaxy. The two galaxies together are also classified as Arp 78 in the

text: Arp peculiar galaxy catalog

text: . NGC 772 has a diameter of 240,000 light-years and the system is 114 million light-years from Earth. Another spiral galaxy in Aries is

text: NGC 673

text: , a face-on class SAB(s)c galaxy. It is a weakly

text: barred spiral galaxy

text: with loosely wound arms. It has no ring and a faint bulge and is 2.5 by 1.9 arcminutes. It has two primary arms with fragments located farther from the core. 171,000 light-years in diameter, NGC 673 is 235 million light-years from Earth.

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answers: 0: The answer is not relevant or complete at all.

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answers: loosely wound arms

answers: NDQ_002602

answers: spiral galaxy

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answers: elliptical galaxy

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answers: spiral arms that are wound somewhat tightly

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answers: star forming regions

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answers: ellipticity

answers: NDQ_002607

answers: Arietis

answers: NDQ_002609

answers: 3 billion stars

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answers: ring

answers: NDQ_002612

answers: spiral galaxy

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answers: star forming regions

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answers: ellipticity

answers: NDQ_002618

answers: The Milky Way

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answers: companion galaxy

answers: NDQ_002620

answers: class SA(s)b galaxy

answers: NDQ_002621

answers: galaxy

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answers: The main arm

answers: NDQ_002623

answers: elliptical

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answers: face-on

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answers: Milky Way Galaxy

answers: NDQ_002626

answers: Gravitational interactions

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answers: galaxy

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answers: companion galaxy

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answers: open star clusters

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answers: class SA(s)b galaxy

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answers: It is a relatively bright galaxy

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answers: NGC 770

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answers: galaxy

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answers: The main arm

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answers: Earth

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answers: NGC 772

text: The stars within an asterism rarely have any substantial astrophysical relationship to each other, and their apparent proximity when viewed from Earth disguises the fact that they are far apart, some being much farther from Earth than others. However, there are some exceptions: almost all of the stars in the constellation of Ursa Major (including most of the Big Dipper) are genuinely close to one another, travel through the galaxy with similar velocities, and are likely to have formed together as part of a cluster that is slowly dispersing. These stars form the Ursa Major moving group.

text: The stars within an asterism rarely have any substantial astrophysical relationship to each other, and their apparent proximity when viewed from Earth disguises the fact that they are far apart, some being much farther from Earth than others. However, there are some exceptions: almost all of the stars in the constellation of Ursa Major (including most of the Big Dipper) are genuinely close to one another, travel through the galaxy with similar

text: velocities

text: , and are likely to have formed together as part of a

text: cluster

text: that is slowly dispersing. These stars form the

text: Ursa Major moving group

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answers: moving group

answers: NDQ_002599

answers: galaxy

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answers: stars

answers: NDQ_002601

answers: asterism

answers: NDQ_002602

answers: cluster

answers: NDQ_002603

answers: they are far apart

answers: NDQ_002604

answers: far apart

answers: NDQ_002605

answers: far apart

answers: NDQ_002606

answers: asterism

answers: NDQ_002607

answers: form the Ursa Major moving group

answers: NDQ_002609

answers: 4 billion stars

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answers: cluster

answers: NDQ_002612

answers: galaxy

answers: NDQ_002615

answers: moving group

answers: NDQ_002617

answers: asterism

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: asterism

answers: NDQ_002620

answers: stars in the constellation of Ursa Major

answers: NDQ_002621

answers: cluster

answers: NDQ_002622

answers: moving group

answers: NDQ_002623

answers: stars within an asterism rarely have any substantial astrophysical relationship to each other

answers: NDQ_002624

answers: asterism

answers: NDQ_002625

answers: the Milky Way Galaxy

answers: NDQ_002626

answers: Earth is rotating around our galaxy.

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: galaxy

answers: NDQ_002631

answers: Spiral

answers: NDQ_002632

answers: dwarf galaxies are often found near larger galaxies

answers: NDQ_002633

answers: galaxy

answers: NDQ_002634

answers: Stars within an asterism

answers: NDQ_002635

answers: Earth orbits the central disk of our galaxy.

answers: NDQ_002636

answers: Stars within an asterism

text: The Northern Local Supervoid is a region of space devoid of rich clusters of galaxies, known as a void. It is the closest supervoid and is located between the Virgo (Local), Coma and Hercules superclusters. On the sky, it is located between Boötes, Virgo, and Serpens Caput constellations. It contains a few small galaxies (primarily spirals) and galaxy clusters, but is mostly empty. The faint galaxies within this void divide the region into smaller voids, which are 3–10 times smaller than the supervoid. The center is located  away at approximately (, ) and it is  in diameter across its narrowest width.

text: The Northern Local Supervoid is a region of space devoid of rich clusters of

text: galaxies

text: , known as a

text: void

text: . It is the closest supervoid and is located between the

text: Virgo

text: (Local),

text: Coma

text: and

text: Hercules

text: supercluster

text: s. On the sky, it is located between

text: Boötes

text: Virgo

text: , and

text: Serpens Caput

text: constellation

text: s. It contains a few small

text: galaxies

text: (primarily

text: spirals

text: ) and galaxy clusters, but is mostly empty. The faint galaxies within this void divide the region into smaller voids, which are 3–10 times smaller than the supervoid. The center is located  away at approximately (, ) and it is  in diameter across its narrowest width.

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answers: galaxy clusters

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answers: 3–10 times smaller

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answers: empty

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answers: a few small galaxies

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answers: The Milky Way Galaxy

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answers: The center is located away at approximately (, ) and it is in diameter across its narrowest width

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answers: It contains a few small galaxies

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answers: galaxy clusters

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answers: Open star clusters

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answers: small galaxies

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answers: spiral galaxies

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answers: It contains a few small galaxies

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answers: Rich clusters of galaxies

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answers: Virgo (Local)

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answers: The center is located away at approximately

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answers: It contains a few small galaxies

text: Globular clusters, which are found in the halo of a galaxy, contain considerably more stars and are much older than the less dense galactic, or open clusters, which are found in the disk. Globular clusters are fairly common; there are about 150 to 158 currently known globular clusters in the Milky Way, with perhaps 10 to 20 more still undiscovered. These globular clusters orbit the Galaxy at radii of 40 kiloparsecs (130,000 light-years) or more. Larger galaxies can have more: Andromeda Galaxy, for instance, may have as many as 500. Some giant elliptical galaxies (particularly those at the centers of galaxy clusters) such as M87, have as many as 13,000 globular clusters.

text: Globular clusters, which are found in the

text: halo

text: of a

text: galaxy

text: , contain considerably more stars and are much older than the less dense

text: galactic, or open cluster

text: s, which are found in the disk. Globular clusters are fairly common; there are about 150 to 158 currently known globular clusters in the

text: Milky Way

text: , with perhaps 10 to 20 more still undiscovered. These globular clusters orbit the Galaxy at radii of 40

text: kiloparsecs

text: light-year

text: s) or more. Larger galaxies can have more:

text: Andromeda Galaxy

text: , for instance, may have as many as 500. Some giant

text: elliptical galaxies

text: (particularly those at the centers of

text: galaxy cluster

text: s) such as

text: , have as many as 13,000 globular clusters.

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answers: open clusters

answers: NDQ_002599

answers: as many as 500

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answers: globular clusters

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answers: elliptical

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answers: the Milky Way

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answers: disk

answers: NDQ_002604

answers: halo

answers: NDQ_002605

answers: less dense

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answers: open clusters

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answers: are found in the halo of a galaxy

answers: NDQ_002609

answers: 150 to 158

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answers: globular clusters

answers: NDQ_002612

answers: Milky Way

answers: NDQ_002615

answers: globular clusters

answers: NDQ_002617

answers: elliptical

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answers: 130,000 light-years

answers: NDQ_002619

answers: open clusters

answers: NDQ_002620

answers: Globular clusters

answers: NDQ_002621

answers: clusters

answers: NDQ_002622

answers: Globular clusters

answers: NDQ_002623

answers: Galaxy clusters

answers: NDQ_002624

answers: halo

answers: NDQ_002625

answers: Galaxy

answers: NDQ_002626

answers: orbit the Galaxy at radii of 40 kiloparsecs

answers: NDQ_002627

answers: The Milky Way, with perhaps 10 to 20 more still undiscovered

answers: NDQ_002628

answers: Galaxy clusters

answers: NDQ_002629

answers: Globular clusters

answers: NDQ_002630

answers: Globular clusters

answers: NDQ_002631

answers: Globular clusters

answers: NDQ_002632

answers: Smaller galaxies

answers: NDQ_002633

answers: Larger galaxies can have more

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answers: Galaxy

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answers: The Milky Way

answers: NDQ_002636

answers: Milky Way

text: The Circinus Galaxy (ESO 97-G13) is a Seyfert galaxy in the Circinus constellation.  It is located 4 degrees below the Galactic plane, and, at a distance of 13 million light-years, it is one of the closest to the Milky Way.  The galaxy is undergoing tumultuous changes, as rings of gas are being ejected from the galaxy.  The outermost ring is 700 light-years from the center of the galaxy and the inner ring is 130 light-years out.  Although the Circinus galaxy  can be seen using a small telescope, it was not noticed until 1977 because it lies close to the plane of the Milky Way and is obscured by galactic dust.  The Circinus Galaxy is a Type II Seyfert galaxy and is one of the closest known active galaxies to the Milky Way, though it is probably slightly further away than Centaurus A.

text: The Circinus Galaxy (ESO 97-G13) is a

text: Seyfert galaxy

text: in the

text: Circinus constellation

text: .  It is located 4 degrees below the

text: Galactic plane

text: , and, at a distance of 13 million

text: light-year

text: s, it is one of the closest to the

text: Milky Way

text: .  The galaxy is undergoing tumultuous changes, as rings of gas are being ejected from the galaxy.  The outermost ring is 700 light-years from the center of the galaxy and the inner ring is 130 light-years out.  Although the Circinus galaxy  can be seen using a small telescope, it was not noticed until 1977 because it lies close to the plane of the Milky Way and is obscured by galactic dust.  The Circinus Galaxy is a Type II

text: Seyfert galaxy

text: and is one of the closest known

text: active galaxies

text: to the

text: Milky Way

text: , though it is probably slightly further away than

text: Centaurus A

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text: Along the pathway are thirteen markers denoting the passage of each billion years. At eight landings, panels show visitors the relative size of the universe at that point in time, along with major developmental stages of the universe including the first generation of stars, globular clusters, quasars, elliptical galaxies, galactic bulges, radio galaxies, the Milky Way Galaxy, galactic disks, and later generations of stars. At each of the landings, computer interactives provide overviews of the entire pathway, and more in-depth information, as well as connections to exhibit topics in the Hall of the Universe.

text: Along the pathway are thirteen markers denoting the passage of each billion years. At eight landings, panels show visitors the relative size of the universe at that point in time, along with major developmental stages of the universe including the first generation of stars,

text: globular clusters

text: quasar

text: s,

text: elliptical galaxies

text: galactic bulges

text: radio galaxies

text: , the

text: Milky Way Galaxy

text: galactic disk

text: s, and later generations of stars. At each of the landings, computer interactives provide overviews of the entire pathway, and more in-depth information, as well as connections to exhibit topics in the Hall of the Universe.

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text: Examples of chaotic rotation include Hyperion, a moon of Saturn which rotates so unpredictably that the Cassini probe could not be reliably scheduled to pass by unexplored regions, and Pluto's Nix, Hydra, and possibly Styx and Kerberos. According to Mark R. Snowalter, author of a recent study, "Nix can flip its entire pole. It could actually be possible to spend a day on Nix in which the sun rises in the east and sets in the north. It is almost random-looking in the way it rotates." Another example is that of galaxies; from careful observation by the Keck and Hubble Telescopes of hundreds of galaxies, a trend was discovered that suggests galaxies such as our own Milky Way used to have a very chaotic rotation, with planetary bodies and stars rotating randomly. New evidence suggests that our galaxy and other have settled into an orderly, disk-like rotation over the past 8 million years and that other galaxies are slowly following suit over time.

text: Examples of chaotic rotation include

text: Hyperion

text: , a moon of

text: Saturn

text: which rotates so unpredictably that the

text: Cassini probe

text: could not be reliably scheduled to pass by unexplored regions, and

text: Pluto's

text: Nix

text: Hydra

text: , and possibly

text: Styx

text: and

text: Kerberos

text: . According to Mark R. Snowalter, author of a recent study, "Nix can flip its entire pole. It could actually be possible to spend a day on Nix in which the sun rises in the east and sets in the north. It is almost random-looking in the way it rotates." Another example is that of

text: galaxies

text: ; from careful observation by the

text: Keck

text: and

text: Hubble Telescopes

text: of hundreds of galaxies, a trend was discovered that suggests galaxies such as our own

text: Milky Way

text: used to have a very chaotic rotation, with

text: planetary bodies

text: and stars rotating randomly. New evidence suggests that our galaxy and other have settled into an orderly, disk-like rotation over the past 8 million years and that other galaxies are slowly following suit over time.

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text: Tololo-1247-232 (Tol 1247 or T1247)) is a small galaxy at a distance of  (redshift z=0.0480). It is situated in the southern equatorial constellation of Hydra. Visually Tol 1247 appears to be an irregular or possibly a barred spiral galaxy. Tol 1247 is named after the surveys that were carried at the Cerro Tololo Inter-American Observatory (CTIO), the first of which was in 1976. It is one of nine galaxies in the local universe known to emit Lyman Continuum photons (LyC).

text: Tololo-1247-232 (Tol 1247 or T1247)) is a small

text: galaxy

text: at a distance of  (

text: redshift

text: z=0.0480). It is situated in the southern equatorial constellation of

text: Hydra

text: . Visually Tol 1247 appears to be an irregular or possibly a barred spiral galaxy. Tol 1247 is named after the surveys that were carried at the

text: Cerro Tololo Inter-American Observatory

text: (CTIO), the first of which was in 1976. It is one of nine galaxies in the local universe known to emit

text: Lyman Continuum photons

text: (LyC).

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text: Elliptical galaxies are preferentially found in galaxy clusters and in compact groups of galaxies.

text: Elliptical galaxies are preferentially found in

text: galaxy clusters

text: and in compact

text: groups of galaxies

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text: The prominent open cluster the Pleiades has been recognized as a group of stars since antiquity, while the Hyades forms part of Taurus, one of the oldest constellations. Other open clusters were noted by early astronomers as unresolved fuzzy patches of light. The Roman astronomer Ptolemy mentions the Praesepe, the Double Cluster in Perseus, and the Ptolemy Cluster, while the Persian astronomer Al-Sufi wrote of the Omicron Velorum cluster. However, it would require the invention of the telescope to resolve these nebulae into their constituent stars. Indeed, in 1603 Johann Bayer gave three of these clusters designations as if they were single stars.

text: The prominent open cluster the Pleiades has been recognized as a group of stars since antiquity, while the Hyades forms part of

text: Taurus

text: , one of the oldest constellations. Other open clusters were noted by early astronomers as unresolved fuzzy patches of light. The Roman astronomer

text: Ptolemy

text: mentions the

text: Praesepe

text: , the

text: Double Cluster

text: in

text: Perseus

text: , and the

text: Ptolemy Cluster

text: , while the Persian astronomer

text: Al-Sufi

text: wrote of the

text: Omicron Velorum cluster

text: . However, it would require the invention of the

text: telescope

text: to resolve these nebulae into their constituent stars. Indeed, in 1603

text: Johann Bayer

text: gave three of these clusters

text: designations

text: as if they were single stars.

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answers: It would require the invention of the telescope

text: These two populations have been observed in many galaxies, especially massive elliptical galaxies. Both groups are nearly as old as the universe itself and are of similar ages, but differ in their metal abundances. Many scenarios have been suggested to explain these subpopulations, including violent gas-rich galaxy mergers, the accretion of dwarf galaxies, and multiple phases of star formation in a single galaxy. In the Milky Way, the metal-poor clusters are associated with the halo and the metal-rich clusters with the bulge.

text: These two populations have been observed in many galaxies, especially massive

text: elliptical galaxies

text: . Both groups are nearly as old as the universe itself and are of similar ages, but differ in their metal abundances. Many scenarios have been suggested to explain these subpopulations, including violent gas-rich galaxy mergers, the accretion of dwarf galaxies, and multiple phases of star formation in a single galaxy. In the

text: Milky Way

text: , the metal-poor clusters are associated with the halo and the metal-rich clusters with the bulge.

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answers: metal-poor clusters

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answers: galaxies

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answers: violent gas-rich galaxy mergers

answers: NDQ_002602

answers: massive elliptical

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answers: metal-poor

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answers: metal-poor

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answers: metal-rich

answers: NDQ_002606

answers: dwarf galaxies

answers: NDQ_002607

answers: metal-poor clusters are associated with the halo

answers: NDQ_002609

answers: 1 billion stars

answers: NDQ_002610

answers: bulge

answers: NDQ_002612

answers: Milky Way

answers: NDQ_002615

answers: dwarf

answers: NDQ_002617

answers: elliptical

answers: NDQ_002618

answers: The Milky Way

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answers: dwarf

answers: NDQ_002620

answers: The Milky Way

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: dwarf galaxies

answers: NDQ_002623

answers: metal-poor clusters

answers: NDQ_002624

answers: dwarf

answers: NDQ_002625

answers: Milky Way

answers: NDQ_002626

answers: The Milky Way

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answers: The Milky Way

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answers: galaxy

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answers: globular star clusters

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answers: massive

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answers: spiral galaxies

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answers: The Milky Way

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answers: The Milky Way

answers: NDQ_002634

answers: In the Milky Way

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answers: The Milky Way

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answers: Milky Way

text: The municipalities of Liechtenstein, the Gemeinden, exhibit complex shapes, despite their small size.

text: The municipalities of Liechtenstein, the Gemeinden, exhibit complex shapes, despite their small size.

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answers: complex shapes

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answers: many stars

answers: NDQ_002600

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answers: complex shapes

answers: NDQ_002602

answers: complex shapes

answers: NDQ_002603

answers: complex shapes

answers: NDQ_002604

answers: complex shapes

answers: NDQ_002605

answers: complex shapes

answers: NDQ_002606

answers: complex shapes

answers: NDQ_002607

answers: globular clusters

answers: NDQ_002609

answers: billions of stars

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answers: galaxy

answers: NDQ_002612

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answers: NDQ_002615

answers: Gemeinden

answers: NDQ_002617

answers: Liechtenstein

answers: NDQ_002618

answers: The Milky Way

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answers: Gemeinden

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answers: dwarf

answers: NDQ_002621

answers: Liechtenstein

answers: NDQ_002622

answers: Gemeinden

answers: NDQ_002623

answers: Liechtenstein

answers: NDQ_002624

answers: Liechtenstein

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is rotating around our galaxy.

answers: NDQ_002627

answers: The municipalities of Liechtenstein

answers: NDQ_002628

answers: Star clusters

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answers: Open star clusters

answers: NDQ_002630

answers: Small

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answers: elliptical

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answers: larger galaxies

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answers: Our solar system is within one of the spiral arms

answers: NDQ_002635

answers: Our solar system orbits the central disk

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answers: complex shapes

text: H II regions can be seen to considerable distances in the universe, and the study of extragalactic H II regions is important in determining the distance and chemical composition of galaxies. Spiral and irregular galaxies contain many H II regions, while elliptical galaxies are almost devoid of them. In spiral galaxies, including our Milky Way, H II regions are concentrated in the spiral arms, while in irregular galaxies they are distributed chaotically. Some galaxies contain huge H II regions, which may contain tens of thousands of stars. Examples include the 30 Doradus region in the Large Magellanic Cloud and NGC 604 in the Triangulum Galaxy.

text: H II regions can be seen to considerable distances in the universe, and the study of extragalactic H II regions is important in determining the distance and chemical composition of

text: galaxies

text: Spiral

text: and

text: irregular

text: galaxies contain many H II regions, while

text: elliptical

text: galaxies are almost devoid of them. In spiral galaxies, including our

text: Milky Way

text: , H II regions are concentrated in the

text: spiral arm

text: s, while in irregular galaxies they are distributed chaotically. Some galaxies contain huge H II regions, which may contain tens of thousands of stars. Examples include the

text: 30 Doradus

text: region in the

text: Large Magellanic Cloud

text: and

text: NGC 604

text: in the

text: Triangulum Galaxy

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text: In astronomy, it is widely accepted that most stars are born within molecular clouds known as stellar nurseries. The stars formed within such a cloud compose open clusters containing dozens to thousands of members. These clusters dissociate over time. Stars that separate themselves from the cluster's core are designated as members of the cluster's stellar association. If the remnant later drifts through the Milky Way as a coherent assemblage, then it is termed a moving group.

text: In

text: astronomy

text: , it is widely accepted that most stars are born within molecular clouds known as

text: stellar nurseries

text: . The stars formed within such a cloud compose

text: open cluster

text: s containing dozens to thousands of members. These clusters dissociate over time. Stars that separate themselves from the cluster's core are designated as members of the cluster's stellar association. If the remnant later drifts through the Milky Way as a coherent assemblage, then it is termed a moving group.

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answers: NDQ_002624

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text: Studies from RAVE either concentrate on peculiar stars and objects or overall trends for the different components of our Galaxy, with a main focus of the structure and formation of the Milky Way. For example, RAVE is suited to searching for stellar streams, some of which are remnants of dwarf galaxies that merged with the Milky Way during galaxy formation. A search for a stellar stream from the Sagittarius Dwarf Elliptical Galaxy - which is currently merging with the Milky Way - in the vicinity of the sun yielded a null result, which helps constrain the shape of the Milky Way's dark halo. Another study of the highest velocity stars was used to constrain the local Galactic escape velocity and so the mass of the dark halo.

text: Studies from RAVE either concentrate on peculiar stars and objects or overall trends for the different components of our Galaxy, with a main focus of the structure and formation of the Milky Way. For example, RAVE is suited to searching for

text: stellar streams

text: , some of which are remnants of

text: dwarf galaxies

text: that merged with the Milky Way during

text: galaxy formation

text: . A search for a stellar stream from the

text: Sagittarius Dwarf Elliptical Galaxy

text: - which is currently merging with the Milky Way - in the vicinity of the sun yielded a

text: null result

text: , which helps constrain the shape of the Milky Way's

text: dark halo

text: . Another study of the highest velocity stars was used to constrain the local Galactic

text: escape velocity

text: and so the

text: mass

text: of the dark halo.

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text: The Hubble Space Telescope has been used to provide convincing observational evidence of this stellar mass-sorting process in globular clusters. Heavier stars slow down and crowd at the cluster's core, while lighter stars pick up speed and tend to spend more time at the cluster's periphery. The globular star cluster 47 Tucanae, which is made up of about 1 million stars, is one of the densest globular clusters in the Southern Hemisphere. This cluster was subjected to an intensive photographic survey, which allowed astronomers to track the motion of its stars. Precise velocities were obtained for nearly 15,000 stars in this cluster.

text: The Hubble Space Telescope has been used to provide convincing observational evidence of this stellar mass-sorting process in globular clusters. Heavier stars slow down and crowd at the cluster's core, while lighter stars pick up speed and tend to spend more time at the cluster's periphery. The globular star cluster

text: 47 Tucanae

text: , which is made up of about 1 million stars, is one of the densest globular clusters in the Southern Hemisphere. This cluster was subjected to an intensive photographic survey, which allowed astronomers to track the motion of its stars. Precise velocities were obtained for nearly 15,000 stars in this cluster.

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text: An intermediate spiral galaxy is a galaxy that is in between the classifications of a barred spiral galaxy and an unbarred spiral galaxy. It is designated as SAB in the galaxy morphological classification scheme. By definition, a galaxy is a congregation of stars held together by gravity. The first intermediate spiral galaxy discovered is the Milky Way, by Galileo, in 1610. He was the first person with a telescope powerful enough to make such a discovery. Before Galileo, it was thought that all bright objects in the sky were either the planets in the Solar System, moons, comets, or stars. Until the beginning on the twentieth century, astronomers did not know the size of the Universe, but speculated it to be about as big as the Milky Way. In 1920, at the National Academy of Science, there was a big debate between Harlow Shapley and Heber D. Curtis on whether nebulae are small globular clusters surrounding the Milky Way, or separate galaxies located farther away. Nothing was resolved at the debate; neither side was able to provide conclusive evidence to prove their side correct over their opponent. In 1923, Edwin Hubble resolved the matter with a photograph that he took of the Andromeda Galaxy. What he found in his photograph was a very bright light source pulsing at a certain rate, a Cepheid variable, located outside the Milky Way. This can be used to determine the distance to it. Hubble proved that the Universe was full of galaxies, and disproved that the Milky Way was the extent of the Universe. There are many types of galaxies in the Universe, elliptical, barred spiral galaxies; they vary in shape and size, but on average spiral galaxies are the most abundant.

text: An intermediate spiral galaxy is a galaxy that is in between the classifications of a

text: barred spiral galaxy

text: and an

text: unbarred spiral galaxy

text: . It is designated as SAB in the

text: galaxy morphological classification

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answers: NDQ_002598

answers: globular

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answers: on average spiral galaxies

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answers: stars

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answers: they vary in shape and size

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answers: barred spiral galaxy

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answers: barred spiral galaxy

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answers: stars

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answers: unbarred

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answers: elliptical

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answers: nebulae

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answers: stars

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answers: nebulae

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answers: galaxy

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answers: globular clusters

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answers: elliptical

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answers: galaxy

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answers: globular cluster

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answers: on average spiral galaxies

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answers: galaxy

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answers: galaxy

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answers: It is designated as SAB

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answers: SAB

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answers: Galileo, in 1610

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answers: The Milky Way

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answers: On average spiral galaxies are the most abundant

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answers: galaxy

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answers: open star clusters

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answers: They vary in shape and size

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answers: On average spiral galaxies are the most abundant

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answers: Small globular clusters

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answers: galaxy

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answers: The Milky Way

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answers: The Solar System

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answers: The Milky Way

text: He specializes in the study of star clusters and galaxies.

text: He specializes in the study of

text: star clusters

text: and

text: galaxies

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answers: billions of stars

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answers: Milky Way Galaxy

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answers: Our solar system is rotating around our galaxy.

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answers: Our solar system orbits the center of our galaxy.

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answers: galaxy

text: De Vaucouleurs also assigned numerical values to each class of galaxy in his scheme. Values of the numerical Hubble stage T run from −6 to +10, with negative numbers corresponding to early-type galaxies (ellipticals and lenticulars) and positive numbers to late types (spirals and irregulars). Elliptical galaxies are divided into three 'stages': compact ellipticals (cE), normal ellipticals (E) and late types (E). Lenticulars are similarly subdivided into early (S), intermediate (S) and late (S) types. Irregular galaxies can be of type magellanic irregulars (T = 10) or 'compact' (T = 11).

text: De Vaucouleurs also assigned numerical values to each class of galaxy in his scheme. Values of the numerical Hubble stage T run from −6 to +10, with negative numbers corresponding to early-type galaxies (ellipticals and lenticulars) and positive numbers to late types (spirals and irregulars). Elliptical galaxies are divided into three 'stages': compact ellipticals (cE), normal ellipticals (E) and late types (E). Lenticulars are similarly subdivided into early (S), intermediate (S) and late (S) types. Irregular galaxies can be of type magellanic irregulars (T = 10) or 'compact' (T = 11).

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answers: The solar system is rotating around our galaxy.

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answers: Open star clusters

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answers: Lenticulars

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answers: Spirals and irregulars

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answers: Smaller galaxies are often found near larger galaxies

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answers: Galaxies

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answers: spirals

text: Throughout most of the 1960s when Pontiac annually captured third place in industry sales, behind Chevrolet and Ford, the Catalina was also often the industry's third best-selling full-sized car behind the first-place Chevrolet Impala and second-place Ford Galaxie 500. The Catalina's success in the low-medium priced field led many competitors to respond with similar products such as the 1961 Chrysler Newport, a less-expensive Chrysler that was priced lower than base models bearing the Chrysler nameplate in recent previous years; and the 1962 Dodge Custom 880 and 1963 Mercury Monterey, both of which were introduced as full-fledged low-medium priced full-sized cars in size and power that followed unsuccessful efforts by Mercury and Dodge to bring out downsized full-sized cars.

text: Throughout most of the 1960s when Pontiac annually captured third place in industry sales, behind Chevrolet and Ford, the Catalina was also often the industry's third best-selling full-sized car behind the first-place

text: Chevrolet Impala

text: and second-place

text: Ford Galaxie 500

text: . The Catalina's success in the low-medium priced field led many competitors to respond with similar products such as the 1961

text: Chrysler Newport

text: , a less-expensive Chrysler that was priced lower than base models bearing the Chrysler nameplate in recent previous years; and the 1962

text: Dodge Custom 880

text: and 1963

text: Mercury Monterey

text: , both of which were introduced as full-fledged low-medium priced full-sized cars in size and power that followed unsuccessful efforts by Mercury and Dodge to bring out downsized full-sized cars.

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answers: Galaxie

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answers: Galaxie

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answers: The Catalina

answers: NDQ_002627

answers: Galaxie 500

answers: NDQ_002628

answers: Galaxie

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text: Different types of galaxies have different histories of star formation and hence planet formation. Planet formation is affected by the ages, metallicities, and orbits of stellar populations within a galaxy. Distribution of stellar populations within a galaxy varies between the different types of galaxies.Stars in elliptical galaxies are much older than stars in spiral galaxies. Most elliptical galaxies contain mainly low-mass stars, with minimal star-formation activity. The distribution of the different types of galaxies in the universe depends on their location within galaxy clusters, with elliptical galaxies found mostly close to their centers.

text: Different

text: types of galaxies

text: have different histories of

text: star formation

text: and hence

text: planet formation

text: . Planet formation is affected by the ages, metallicities, and orbits of stellar populations within a galaxy. Distribution of stellar populations within a galaxy varies between the different types of galaxies.Stars in

text: elliptical galaxies

text: are much older than stars in

text: spiral galaxies

text: . Most elliptical galaxies contain mainly

text: low-mass stars

text: , with minimal

text: star-formation

text: activity. The distribution of the different types of galaxies in the

text: universe

text: depends on their location within

text: galaxy cluster

text: s, with elliptical galaxies found mostly close to their centers.

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answers: galaxy clusters

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answers: They contain mainly low-mass stars, with minimal star-formation activity

answers: NDQ_002624

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answers: Milky Way Galaxy

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answers: orbits of stellar populations

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answers: Stars in elliptical galaxies are much older

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text: The Tucana Dwarf galaxy is one of only two dwarf spheroidal galaxies in the Local Group  not located near the Milky Way or the Andromeda Galaxy. It is therefore likely to have evolved in isolation for most of its history.

text: The Tucana Dwarf galaxy is one of only two dwarf spheroidal galaxies in the Local Group  not located near the Milky Way or the

text: Andromeda Galaxy

text: . It is therefore likely to have evolved in isolation for most of its history.

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answers: 2: The answer has limited relevance and completeness, with significant gaps or inaccuracy.

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answers: galaxies

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answers: The Milky Way Galaxy

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answers: The Milky Way or the Andromeda Galaxy

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answers: Milky Way

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answers: Milky Way

text: As most galaxies of this type are present in rich galaxy clusters, it has been proposed that this may be one of the reasons that converts normal spirals into anemic ones. Studies of spiral galaxies in the nearby Virgo cluster have shown not only how, unlike in isolated spiral galaxies, in most cases their neutral gas and star formation are truncated within their optical disks, in some cases quite severely, but also how star formation activity in them is lower than on spirals outside clusters,: this means that processes that take place in galaxy clusters as interactions with the intracluster medium like ram-pressure stripping and/or interactions with other neighboring galaxies are responsible of the origin of anemic galaxies, stripping the normal spirals of their gas, increasing in some cases their star formation activity, and thus in the end quenching the latter as their gas is exhausted and not replenished. Spiral galaxies may have become anemic ones by exhausting their supply of gas via star formation activity.

text: As most galaxies of this type are present in rich

text: galaxy cluster

text: s, it has been proposed that this may be one of the reasons that converts normal spirals into anemic ones. Studies of spiral galaxies in the nearby

text: Virgo cluster

text: have shown not only how, unlike in isolated spiral galaxies, in most cases their neutral gas and star formation are truncated within their optical disks, in some cases quite severely, but also how star formation activity in them is lower than on spirals outside clusters,: this means that processes that take place in galaxy clusters as interactions with the

text: intracluster medium

text: like

text: ram-pressure stripping

text: and/or

text: interactions with other neighboring galaxies

text: are responsible of the origin of anemic galaxies, stripping the normal spirals of their gas, increasing in some cases their star formation activity, and thus in the end quenching the latter as their gas is exhausted and not replenished. Spiral galaxies may have become anemic ones by exhausting their supply of gas via star formation activity.

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answers: open star clusters

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answers: As most galaxies of this type are present in rich galaxy clusters

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answers: Virgo

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text: Studies say that a triple-star system was traveling through the center of the Milky Way when it came too close to the galactic center (which is thought to have a giant black hole). One of the stars was captured by the black hole causing the other two to be ejected from the Milky Way, where they merged to form a hot blue star. The star is moving at a speed of , about three times faster than the Sun's orbital velocity around the galaxy's center, and also faster than the galaxy's escape velocity.

text: Studies say that a triple-star system was traveling through the center of the

text: Milky Way

text: when it came too close to the galactic center (which is thought to have a giant

text: black hole

text: ). One of the stars was captured by the black hole causing the other two to be ejected from the

text: Milky Way

text: , where they merged to form a hot blue star. The star is moving at a speed of , about three times faster than the

text: Sun

text: 's orbital velocity around the

text: galaxy

text: 's center, and also faster than the galaxy's

text: escape velocity

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answers: orbital velocity around the galaxy's center, and also faster than the galaxy's escape velocity

answers: NDQ_002627

answers: The Milky Way

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answers: Open star clusters

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answers: Milky Way

text: Astronomers have estimated the Milky Way galaxy, will collide with the Andromeda galaxy in about 4.5 billion years. It is thought that the two spiral galaxies will eventually merge to become an elliptical galaxy or perhaps a large disk galaxy.

text: Astronomers have estimated the

text: Milky Way galaxy

text: , will collide with the

text: Andromeda galaxy

text: in about 4.5 billion years. It is thought that the two

text: spiral galaxies

text: will eventually merge to become an

text: elliptical galaxy

text: or perhaps a large

text: disk galaxy

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answers: The Milky Way galaxy is a spiral galaxy.

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answers: The Milky Way galaxy is the largest galaxy in the universe.

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text: Various morphological features of galaxies can affect their potential for habitability. Spiral arms, for example, are the location of star formation, but they contain numerous giant molecular clouds and a high density of stars that can perturb a star's Oort cloud, sending avalanches of comets and asteroids toward any planets further in. In addition, the high density of stars and rate of massive star formation can expose any stars orbiting within the spiral arms for too long to supernova explosions, reducing their prospects for the survival and development of life. Considering these factors, the Sun is advantageously placed within the galaxy because, in addition to being outside a spiral arm, it orbits near the corotation radius, maximizing the interval between spiral-arm crossings.

text: Various morphological features of galaxies can affect their potential for habitability. Spiral arms, for example, are the location of star formation, but they contain numerous giant molecular clouds and a high density of stars that can perturb a star's

text: Oort cloud

text: , sending avalanches of comets and asteroids toward any planets further in. In addition, the high density of stars and rate of massive star formation can expose any stars orbiting within the spiral arms for too long to supernova explosions, reducing their prospects for the survival and development of life. Considering these factors, the

text: Sun

text: is advantageously placed within the galaxy because, in addition to being outside a spiral arm, it orbits near the

text: corotation radius

text: , maximizing the interval between spiral-arm crossings.

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answers: The Sun is advantageously placed

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answers: Spiral arms

text: These new-found star clusters contain hundreds of thousands of stars, a similar number of stars that can be found in globular clusters. The clusters also share other characteristics with globular clusters, e.g. the stellar populations and metallicity. What distinguishes them from the globular clusters is that they are much larger – several hundred light-years across – and hundreds of times less dense. The distances between the stars are, therefore, much greater within the newly discovered extended clusters. Parametrically, these clusters lie somewhere between a (low dark matter) globular cluster and a (dark matter-dominated) dwarf spheroidal galaxy.

text: These new-found star clusters contain hundreds of thousands of stars, a similar number of stars that can be found in globular clusters. The clusters also share other characteristics with globular clusters, e.g. the stellar populations and metallicity. What distinguishes them from the globular clusters is that they are much larger – several hundred light-years across – and hundreds of times less dense. The distances between the stars are, therefore, much greater within the newly discovered extended clusters. Parametrically, these clusters lie somewhere between a (low dark matter) globular cluster and a (dark matter-dominated)

text: dwarf spheroidal galaxy

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answers: globular clusters

answers: NDQ_002599

answers: hundreds of thousands

answers: NDQ_002600

answers: Dark matter

answers: NDQ_002601

answers: spheroidal

answers: NDQ_002602

answers: globular clusters

answers: NDQ_002603

answers: Dark matter-dominated

answers: NDQ_002604

answers: hundreds of times less dense

answers: NDQ_002605

answers: low dark matter

answers: NDQ_002606

answers: spheroidal

answers: NDQ_002607

answers: can be found in globular clusters

answers: NDQ_002609

answers: thousands of stars

answers: NDQ_002610

answers: spheroidal galaxy

answers: NDQ_002612

answers: globular cluster

answers: NDQ_002615

answers: globular clusters

answers: NDQ_002617

answers: spheroidal galaxy

answers: NDQ_002618

answers: galaxy

answers: NDQ_002619

answers: star clusters

answers: NDQ_002620

answers: globular clusters

answers: NDQ_002621

answers: star clusters

answers: NDQ_002622

answers: globular clusters

answers: NDQ_002623

answers: globular clusters

answers: NDQ_002624

answers: dwarf spheroidal

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: hundreds of thousands of stars

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answers: globular cluster

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answers: It's impossible to say

answers: NDQ_002632

answers: dwarf spheroidal galaxy

answers: NDQ_002633

answers: globular clusters

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answers: galaxy

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answers: Light-years

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answers: dwarf spheroidal galaxy

text: It has been speculated that Omega Centauri may be the core of a dwarf galaxy that was disrupted and absorbed by the Milky Way. Indeed, Kapteyn's Star, which is currently only 13 light years away, is thought to originate from Omega Centauri. Omega Centauri's chemistry and motion in the Milky Way are also consistent with this picture. Like Mayall II, Omega Centauri has a range of metallicities and stellar ages that suggests that it did not all form at once (as globular clusters are thought to form) and may in fact be the remainder of the core of a smaller galaxy long since incorporated into the Milky Way.

text: It has been speculated that Omega Centauri may be the core of a

text: dwarf galaxy

text: that was disrupted and absorbed by the Milky Way. Indeed,

text: Kapteyn's Star

text: , which is currently only 13 light years away, is thought to originate from Omega Centauri. Omega Centauri's chemistry and motion in the Milky Way are also consistent with this picture. Like Mayall II, Omega Centauri has a range of

text: metallicities

text: and stellar ages that suggests that it did not all form at once (as globular clusters are thought to form) and may in fact be the remainder of the core of a smaller galaxy long since incorporated into the Milky Way.

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answers: 4

answers: NDQ_002598

answers: globular

answers: NDQ_002599

answers: Milky Way

answers: NDQ_002600

answers: Omega Centauri

answers: NDQ_002601

answers: range of metallicities and stellar ages

answers: NDQ_002602

answers: dwarf galaxy

answers: NDQ_002603

answers: Omega Centauri

answers: NDQ_002604

answers: range of metallicities

answers: NDQ_002605

answers: metallicities

answers: NDQ_002606

answers: dwarf galaxy

answers: NDQ_002607

answers: are thought to form

answers: NDQ_002609

answers: 13 light years

answers: NDQ_002610

answers: Omega Centauri

answers: NDQ_002612

answers: Milky Way

answers: NDQ_002615

answers: globular clusters

answers: NDQ_002617

answers: Milky Way

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: dwarf galaxy

answers: NDQ_002620

answers: Milky Way

answers: NDQ_002621

answers: Galaxies

answers: NDQ_002622

answers: globular cluster

answers: NDQ_002623

answers: Kapteyn's Star

answers: NDQ_002624

answers: dwarf galaxy

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: Kapteyn's Star

answers: NDQ_002627

answers: Milky Way

answers: NDQ_002628

answers: globular clusters

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: dwarf galaxy

answers: NDQ_002631

answers: Omega Centauri

answers: NDQ_002632

answers: Milky Way

answers: NDQ_002633

answers: Milky Way

answers: NDQ_002634

answers: Milky Way

answers: NDQ_002635

answers: Milky Way

answers: NDQ_002636

answers: Milky Way

text: The table below lists galaxies that have been consistently identified as group members in the Nearby Galaxies Catalog, the survey of Fouque et al., the Lyons Groups of Galaxies (LGG) Catalog, and the three group lists created from the Nearby Optical Galaxy sample of Giuricin et al.

text: The table below lists galaxies that have been consistently identified as group members in the Nearby Galaxies Catalog, the survey of Fouque et al., the Lyons Groups of Galaxies (LGG) Catalog, and the three group lists created from the Nearby Optical Galaxy sample of Giuricin et al.

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text: It was realised as early as 1767 that the stars in a cluster were physically related, when the English naturalist Reverend John Michell calculated that the probability of even just one group of stars like the Pleiades being the result of a chance alignment as seen from Earth was just 1 in 496,000. Between 1774–1781, French astronomer Charles Messier published a catalogue of celestial objects that had a nebulous appearance similar to comets. This catalogue included 26 open clusters. In the 1790s, English astronomer William Herschel began an extensive study of nebulous celestial objects. He discovered that many of these features could be resolved into groupings of individual stars. Herschel conceived the idea that stars were initially scattered across space, but later became clustered together as star systems because of gravitational attraction. He divided the nebulae into eight classes, with classes VI through VIII being used to classify clusters of stars.

text: It was realised as early as 1767 that the stars in a cluster were physically related, when the English naturalist Reverend

text: John Michell

text: calculated that the probability of even just one group of stars like the Pleiades being the result of a chance alignment as seen from Earth was just 1 in 496,000. Between 1774–1781, French astronomer

text: Charles Messier

text: published a catalogue of celestial objects that had a nebulous appearance similar to

text: comet

text: s. This catalogue included 26 open clusters. In the 1790s, English astronomer

text: William Herschel

text: began an extensive study of nebulous celestial objects. He discovered that many of these features could be resolved into groupings of individual stars. Herschel conceived the idea that stars were initially scattered across space, but later became clustered together as star systems because of gravitational attraction. He divided the nebulae into eight classes, with classes VI through VIII being used to classify clusters of stars.

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answers: It was realised as early as 1767

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text: The Ori order their followers to begin constructing a fleet of ships after learning of the existence of the Milky Way galaxy in . Due to their advanced technology, their ships pose a considerable threat.

text: The

text: Ori

text: order their followers to begin constructing a fleet of ships after learning of the existence of the Milky Way galaxy in . Due to their advanced technology, their ships pose a considerable threat.

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text: In 2004, a team of astronomers focused on the cluster to estimate the age of the Milky Way Galaxy. The team consisted of Luca Pasquini, Piercarlo Bonifacio, Sofia Randich, Daniele Galli, and Raffaele G. Gratton. They used the UV-Visual Echelle Spectrograph of the Very Large Telescope at Cerro Paranal to measure the beryllium content of two stars in the cluster. This allowed them to deduce the time elapsed between the rise of the first generation of stars in the entire Galaxy and the first generation of stars in the cluster. This, added to the estimated age of the stars in the cluster, gives an estimate for the age for the Galaxy: about 13.6 billion years, which is nearly as old as the universe itself.

text: In 2004, a team of

text: astronomer

text: s focused on the cluster to estimate the age of the

text: Milky Way Galaxy

text: . The team consisted of Luca Pasquini, Piercarlo Bonifacio, Sofia Randich, Daniele Galli, and Raffaele G. Gratton. They used the UV-Visual

text: Echelle Spectrograph

text: of the

text: Very Large Telescope

text: at

text: Cerro Paranal

text: to measure the

text: beryllium

text: content of two stars in the cluster. This allowed them to deduce the time elapsed between the rise of the first generation of stars in the entire Galaxy and the first generation of stars in the cluster. This, added to the estimated age of the stars in the cluster, gives an estimate for the age for the Galaxy: about 13.6

text: billion

text: years, which is nearly as

text: old as the universe

text: itself.

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answers: NDQ_002636

answers: Milky Way Galaxy

text: Because most if not all stars form clustered, star clusters are to be viewed the fundamental building blocks of galaxies. The violent gas-expulsion events that shape and destroy many star clusters at birth leave their imprint in the morphological and kinematical structures of galaxies. Most open clusters form with at least 100 stars and a mass of 50 or more solar masses. The largest clusters can have 10 solar masses, with the massive cluster Westerlund 1 being estimated at 5 × 10 solar masses; close to that of a globular cluster. While open clusters and globular clusters form two fairly distinct groups, there may not be a great deal of difference in appearance between a very sparse globular cluster and a very rich open cluster. Some astronomers believe the two types of star clusters form via the same basic mechanism, with the difference being that the conditions that allowed the formation of the very rich globular clusters containing hundreds of thousands of stars no longer prevail in the Milky Way.

text: Because most if not all stars form clustered,

text: star cluster

text: s are to be viewed the fundamental building blocks of galaxies. The violent gas-expulsion events that shape and destroy many star clusters at birth leave their imprint in the morphological and kinematical structures of galaxies. Most open clusters form with at least 100 stars and a mass of 50 or more

text: solar mass

text: es. The largest clusters can have 10 solar masses, with the massive cluster

text: Westerlund 1

text: being estimated at 5 × 10 solar masses; close to that of a globular cluster. While open clusters and globular clusters form two fairly distinct groups, there may not be a great deal of difference in appearance between a very sparse globular cluster and a very rich open cluster. Some astronomers believe the two types of star clusters form via the same basic mechanism, with the difference being that the conditions that allowed the formation of the very rich globular clusters containing hundreds of thousands of stars no longer prevail in the Milky Way.

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answers: NDQ_002598

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answers: NDQ_002599

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answers: NDQ_002600

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answers: NDQ_002601

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answers: NDQ_002602

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answers: NDQ_002603

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answers: NDQ_002604

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answers: NDQ_002605

answers: 4

answers: NDQ_002606

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answers: NDQ_002607

answers: 4

answers: NDQ_002609

answers: 4

answers: NDQ_002610

answers: 4

answers: NDQ_002612

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answers: NDQ_002615

answers: 4

answers: NDQ_002617

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answers: NDQ_002618

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answers: NDQ_002619

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answers: NDQ_002620

answers: 3

answers: NDQ_002621

answers: 4

answers: NDQ_002622

answers: 4

answers: NDQ_002623

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answers: NDQ_002624

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answers: NDQ_002625

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answers: NDQ_002626

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answers: NDQ_002627

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answers: NDQ_002628

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answers: NDQ_002630

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answers: NDQ_002631

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answers: NDQ_002632

answers: 2

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answers: 4

answers: NDQ_002634

answers: 0

answers: NDQ_002635

answers: 0

answers: NDQ_002636

answers: 4

answers: NDQ_002598

answers: globular clusters

answers: NDQ_002599

answers: hundreds of thousands

answers: NDQ_002600

answers: star clusters

answers: NDQ_002601

answers: violent gas-expulsion events

answers: NDQ_002602

answers: Milky Way

answers: NDQ_002603

answers: violent gas-expulsion events

answers: NDQ_002604

answers: star clusters

answers: NDQ_002605

answers: sparse

answers: NDQ_002606

answers: open clusters

answers: NDQ_002607

answers: The largest clusters can have 10 solar masses; close to that of a globular cluster

answers: NDQ_002609

answers: hundreds of thousands of stars

answers: NDQ_002610

answers: globular clusters

answers: NDQ_002612

answers: Milky Way

answers: NDQ_002615

answers: Most open clusters

answers: NDQ_002617

answers: Milky Way

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: open clusters

answers: NDQ_002620

answers: Most open clusters form with at least 100 stars

answers: NDQ_002621

answers: star clusters

answers: NDQ_002622

answers: Westerlund 1

answers: NDQ_002623

answers: galaxies

answers: NDQ_002624

answers: Milky Way

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: The Milky Way

answers: NDQ_002627

answers: The Milky Way

answers: NDQ_002628

answers: galaxies

answers: NDQ_002629

answers: Most open clusters form with at least 100 stars

answers: NDQ_002630

answers: The largest clusters can have 10 solar masses

answers: NDQ_002631

answers: spiral

answers: NDQ_002632

answers: dwarf galaxies are often found near larger galaxies

answers: NDQ_002633

answers: The largest clusters can have 10 solar masses

answers: NDQ_002634

answers: Milky Way

answers: NDQ_002635

answers: Milky Way

answers: NDQ_002636

answers: Milky Way

text: IC 10 is an irregular galaxy that is the only known starburst galaxy in the Local Group of galaxies.

text: IC 10

text: is an irregular galaxy that is the only known

text: starburst galaxy

text: in the Local Group of galaxies.

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answers: 3: The answer has limited relevance and completeness, with noticeable gaps or inaccuracy.

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answers: NDQ_002598

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answers: NDQ_002600

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answers: NDQ_002602

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answers: NDQ_002603

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answers: NDQ_002604

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answers: NDQ_002605

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answers: NDQ_002606

answers: 4

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answers: NDQ_002609

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answers: NDQ_002610

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answers: NDQ_002612

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answers: NDQ_002617

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answers: NDQ_002618

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answers: NDQ_002619

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answers: NDQ_002620

answers: 2

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answers: 4

answers: NDQ_002622

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answers: NDQ_002623

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answers: NDQ_002624

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answers: NDQ_002625

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answers: NDQ_002626

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answers: NDQ_002630

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answers: 2

answers: NDQ_002632

answers: 2

answers: NDQ_002633

answers: 4

answers: NDQ_002634

answers: 0

answers: NDQ_002635

answers: 0

answers: NDQ_002636

answers: 0

answers: NDQ_002598

answers: starburst

answers: NDQ_002599

answers: stars

answers: NDQ_002600

answers: galaxy

answers: NDQ_002601

answers: starburst

answers: NDQ_002602

answers: starburst

answers: NDQ_002603

answers: irregular

answers: NDQ_002604

answers: galaxy

answers: NDQ_002605

answers: galaxies

answers: NDQ_002606

answers: irregular

answers: NDQ_002607

answers: galaxies

answers: NDQ_002609

answers: IC 10

answers: NDQ_002610

answers: starburst

answers: NDQ_002612

answers: starburst

answers: NDQ_002615

answers: galaxy

answers: NDQ_002617

answers: starburst

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: Local Group

answers: NDQ_002620

answers: starburst galaxy

answers: NDQ_002621

answers: Galaxies

answers: NDQ_002622

answers: IC 10

answers: NDQ_002623

answers: irregular

answers: NDQ_002624

answers: irregular galaxy

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: The solar system is rotating around our galaxy.

answers: NDQ_002627

answers: galaxies

answers: NDQ_002628

answers: galaxy

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: irregular

answers: NDQ_002631

answers: irregular

answers: NDQ_002632

answers: Smaller galaxies

answers: NDQ_002633

answers: galaxies

answers: NDQ_002634

answers: IC 10 is an irregular galaxy

answers: NDQ_002635

answers: The solar system orbits the central disk.

answers: NDQ_002636

answers: irregular galaxy

text: Water megamasers were the first type of megamaser discovered. The first water megamaser was found in 1979 in NGC 4945, a galaxy in the nearby Centaurus A/M83 Group. The first hydroxyl megamaser was found in 1982 in Arp 220, which is the nearest ultraluminous infrared galaxy to the Milky Way. All subsequent OH megamasers that have been discovered are also in luminous infrared galaxies, and there are a small number of OH kilomasers hosted in galaxies with lower infrared luminosities. Most luminous infrared galaxies have recently merged or interacted with another galaxy, and are undergoing a burst of star formation. Many of the characteristics of the emission in hydroxyl megamasers are distinct from that of hydroxyl masers within the Milky Way, including the amplification of background radiation and the ratio of hydroxyl lines at different frequencies. The population inversion in hydroxyl molecules is produced by far infrared radiation that results from absorption and re-emission of light from forming stars by surrounding interstellar dust. Zeeman splitting of hydroxyl megamaser lines may be used to measure magnetic fields in the masing regions, and this application represents the first detection of Zeeman splitting in a galaxy other than the Milky Way.

text: Water megamasers were the first type of megamaser discovered. The first water megamaser was found in 1979 in

text: NGC 4945

text: , a galaxy in the nearby

text: Centaurus A/M83 Group

text: . The first hydroxyl megamaser was found in 1982 in

text: Arp 220

text: , which is the nearest

text: ultraluminous infrared galaxy

text: to the Milky Way. All subsequent OH megamasers that have been discovered are also in luminous infrared galaxies, and there are a small number of OH kilomasers hosted in galaxies with lower infrared luminosities. Most luminous infrared galaxies have recently merged or interacted with another galaxy, and are undergoing a burst of

text: star formation

text: . Many of the characteristics of the emission in hydroxyl megamasers are distinct from that of hydroxyl masers within the

text: Milky Way

text: , including the amplification of background radiation and the ratio of hydroxyl lines at different frequencies. The

text: population inversion

text: in hydroxyl molecules is produced by far infrared radiation that results from absorption and re-emission of light from forming stars by surrounding

text: interstellar dust

text: Zeeman splitting

text: of hydroxyl megamaser lines may be used to measure

text: magnetic field

text: s in the masing regions, and this application represents the first detection of Zeeman splitting in a galaxy other than the Milky Way.

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answers: NDQ_002635

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answers: NDQ_002636

answers: 4

answers: NDQ_002598

answers: hydroxyl megamasers

answers: NDQ_002599

answers: Milky Way

answers: NDQ_002600

answers: Milky Way

answers: NDQ_002601

answers: Zeeman splitting

answers: NDQ_002602

answers: Milky Way

answers: NDQ_002603

answers: star formation

answers: NDQ_002604

answers: magnetic fields

answers: NDQ_002605

answers: star formation

answers: NDQ_002606

answers: Milky Way

answers: NDQ_002607

answers: OH kilomasers

answers: NDQ_002609

answers: billions of stars

answers: NDQ_002610

answers: Milky Way

answers: NDQ_002612

answers: Milky Way

answers: NDQ_002615

answers: megamaser

answers: NDQ_002617

answers: Milky Way

answers: NDQ_002618

answers: galaxy

answers: NDQ_002619

answers: A/M83 Group

answers: NDQ_002620

answers: Milky Way

answers: NDQ_002621

answers: galaxy

answers: NDQ_002622

answers: megamaser

answers: NDQ_002623

answers: Most luminous infrared galaxies

answers: NDQ_002624

answers: Milky Way

answers: NDQ_002625

answers: Milky Way

answers: NDQ_002626

answers: The Milky Way

answers: NDQ_002627

answers: galaxy

answers: NDQ_002628

answers: Star clusters

answers: NDQ_002629

answers: open star clusters

answers: NDQ_002630

answers: megamasers

answers: NDQ_002631

answers: Spiral galaxies

answers: NDQ_002632

answers: The Milky Way

answers: NDQ_002633

answers: Milky Way

answers: NDQ_002634

answers: Milky Way

answers: NDQ_002635

answers: Milky Way

answers: NDQ_002636

answers: Milky Way

text: In 2012, a microquasar, a radio burst emanating from a smaller black hole, was detected in the Andromeda Galaxy. The progenitor black hole is located near the galactic center and has about 10 . Discovered through a data collected by the European Space Agency's XMM-Newton probe, and subsequently observed by NASA's Swift Gamma-Ray Burst Mission and Chandra X-Ray Observatory, the Very Large Array, and the Very Long Baseline Array, the microquasar was the first observed within the Andromeda Galaxy and the first outside of the Milky Way Galaxy.

text: In 2012, a

text: microquasar

text: , a radio burst emanating from a smaller black hole, was detected in the Andromeda Galaxy. The progenitor black hole is located near the galactic center and has about 10

text: . Discovered through a data collected by the

text: European Space Agency

text: 's

text: XMM-Newton

text: probe, and subsequently observed by

text: NASA

text: 's

text: Swift Gamma-Ray Burst Mission

text: and

text: Chandra X-Ray Observatory

text: , the

text: Very Large Array

text: , and the

text: Very Long Baseline Array

text: , the microquasar was the first observed within the Andromeda Galaxy and the first outside of the Milky Way Galaxy.

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answers: NDQ_002599

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answers: NDQ_002600

answers: black holes

answers: NDQ_002601

answers: galactic center

answers: NDQ_002602

answers: Milky Way Galaxy

answers: NDQ_002603

answers: black hole

answers: NDQ_002604

answers: black holes

answers: NDQ_002605

answers: galaxy

answers: NDQ_002606

answers: galaxy

answers: NDQ_002607

answers: Black holes

answers: NDQ_002609

answers: 10

answers: NDQ_002610

answers: black hole

answers: NDQ_002612

answers: Milky Way Galaxy

answers: NDQ_002615

answers: Very Large Array

answers: NDQ_002617

answers: Andromeda Galaxy

answers: NDQ_002618

answers: Galaxy

answers: NDQ_002619

answers: quasar

answers: NDQ_002620

answers: Milky Way Galaxy

answers: NDQ_002621

answers: Galaxy

answers: NDQ_002622

answers: Andromeda Galaxy

answers: NDQ_002623

answers: Milky Way Galaxy

answers: NDQ_002624

answers: Andromeda

answers: NDQ_002625

answers: The Milky Way Galaxy

answers: NDQ_002626

answers: Milky Way Galaxy

answers: NDQ_002627

answers: Milky Way Galaxy

answers: NDQ_002628

answers: Galaxy

answers: NDQ_002629

answers: Open star clusters

answers: NDQ_002630

answers: Very Large

answers: NDQ_002631

answers: Andromeda Galaxy

answers: NDQ_002632

answers: Andromeda Galaxy

answers: NDQ_002633

answers: It has about 10.

answers: NDQ_002634

answers: Andromeda Galaxy

answers: NDQ_002635

answers: Milky Way Galaxy

answers: NDQ_002636

answers: Milky Way Galaxy

text: Galaxies undergoing such rapid star formation are known as starburst galaxies. The post-merger elliptical galaxy has a very low gas content, and so H II regions can no longer form. Twenty-first century observations have shown that a very small number of H II regions exist outside galaxies altogether. These intergalactic H II regions may be the remnants of tidal disruptions of small galaxies, and in some cases may represent a new generation of stars in a galaxy's most recently accreted gas.

text: Galaxies undergoing such rapid star formation are known as

text: starburst galaxies

text: . The post-merger elliptical galaxy has a very low gas content, and so H II regions can no longer form. Twenty-first century observations have shown that a very small number of H II regions exist outside galaxies altogether. These intergalactic H II regions may be the remnants of tidal disruptions of small galaxies, and in some cases may represent a new generation of stars in a galaxy's most recently accreted gas.

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answers: H II regions

answers: NDQ_002599

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answers: NDQ_002600

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answers: NDQ_002601

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answers: NDQ_002602

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answers: NDQ_002603

answers: post-merger

answers: NDQ_002604

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answers: NDQ_002605

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answers: NDQ_002606

answers: galaxies

answers: NDQ_002607

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answers: NDQ_002609

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answers: NDQ_002610

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answers: NDQ_002612

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answers: NDQ_002615

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answers: NDQ_002617

answers: elliptical

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: intergalactic

answers: NDQ_002620

answers: Small galaxies

answers: NDQ_002621

answers: Galaxies

answers: NDQ_002622

answers: H II regions

answers: NDQ_002623

answers: H II regions can no longer form

answers: NDQ_002624

answers: starburst galaxies

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Tidal disruptions of small galaxies

answers: NDQ_002627

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answers: NDQ_002628

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answers: NDQ_002629

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answers: NDQ_002630

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answers: NDQ_002631

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answers: NDQ_002632

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answers: NDQ_002633

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answers: NDQ_002635

answers: Galaxies

answers: NDQ_002636

answers: elliptical galaxy

text: DDO 74 (also known as Leo I, Regulus Dwarf, PGC 29488 or UGC 5470) lies approximately 820,000 light years away in the constellation Leo. It is one of the most distant satellite galaxy of our Milky Way. The dwarf spheroidal galaxy is located only 12 arcminutes from Regulus (α Leonis), and the light from Regulus makes the visibility of DDO 74 becomes poor, so it is difficult to be observed.

text: DDO 74

text: (also known as

text: Leo

text: I,

text: Regulus

text: Dwarf

text: PGC

text: 29488 or

text: UGC

text: 5470) lies approximately 820,000

text: light years

text: away in the

text: constellation

text: Leo

text: . It is one of the most distant

text: satellite galaxy

text: of our

text: Milky Way

text: . The

text: dwarf spheroidal galaxy

text: is located only 12 arcminutes from

text: Regulus

text: α Leonis

text: ), and the light from

text: Regulus

text: makes the

text: visibility

text: of

text: DDO 74

text: becomes poor, so it is difficult to be observed.

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answers: DDO 74

answers: NDQ_002609

answers: 820,000 light years

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answers: PGC 29488

answers: NDQ_002617

answers: Milky Way

answers: NDQ_002618

answers: The Milky Way

answers: NDQ_002619

answers: Dwarf

answers: NDQ_002620

answers: Milky Way

answers: NDQ_002621

answers: galaxy

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answers: galaxy

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answers: The dwarf spheroidal galaxy

answers: NDQ_002624

answers: spheroidal

answers: NDQ_002625

answers: Milky Way Galaxy

answers: NDQ_002626

answers: Our solar system is slowly spinning around our galaxy.

answers: NDQ_002627

answers: Milky Way

answers: NDQ_002628

answers: Milky Way

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answers: Open star clusters

answers: NDQ_002630

answers: arcminutes

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answers: DDO 74

answers: NDQ_002632

answers: The dwarf spheroidal galaxy

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answers: Milky Way

answers: NDQ_002634

answers: Milky Way

answers: NDQ_002635

answers: Milky Way

answers: NDQ_002636

answers: Milky Way

text: 2. Weak lensing: where the distortions of background sources are much smaller and can only be detected by analyzing large numbers of sources in a statistical way to find coherent distortions of only a few percent. The lensing shows up statistically as a preferred stretching of the background objects perpendicular to the direction to the center of the lens.By measuring the shapes and orientations of large numbers of distant galaxies, their orientations can be averaged to measure the shear of the lensing field in any region. This, in turn, can be used to reconstruct the mass distribution in the area: in particular, the background distribution of dark matter can be reconstructed. Since galaxies are intrinsically elliptical and the weak gravitational lensing signal is small, a very large number of galaxies must be used in these surveys. These weak lensing surveys must carefully avoid a number of important sources of systematic error: the intrinsic shape of galaxies, the tendency of a camera's point spread function to distort the shape of a galaxy and the tendency of atmospheric seeing to distort images must be understood and carefully accounted for. The results of these surveys are important for cosmological parameter estimation, to better understand and improve upon the Lambda-CDM model, and to provide a consistency check on other cosmological observations. They may also provide an important future constraint on dark energy.

text: Weak lensing

text: : where the distortions of background sources are much smaller and can only be detected by analyzing large numbers of sources in a statistical way to find coherent distortions of only a few percent. The lensing shows up statistically as a preferred stretching of the background objects perpendicular to the direction to the center of the lens.By measuring the shapes and orientations of large numbers of distant galaxies, their orientations can be averaged to measure the

text: shear

text: of the lensing field in any region. This, in turn, can be used to reconstruct the mass distribution in the area: in particular, the background distribution of

text: dark matter

text: can be reconstructed. Since galaxies are intrinsically elliptical and the weak gravitational lensing signal is small, a very large number of galaxies must be used in these surveys. These weak lensing surveys must carefully avoid a number of important sources of

text: systematic error

text: : the intrinsic shape of galaxies, the tendency of a camera's

text: point spread function

text: to distort the shape of a galaxy and the tendency of

text: atmospheric seeing

text: to distort images must be understood and carefully accounted for. The results of these surveys are important for cosmological parameter estimation, to better understand and improve upon the

text: Lambda-CDM model

text: , and to provide a consistency check on other cosmological observations. They may also provide an important future constraint on

text: dark energy

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answers: NDQ_002599

answers: very large number

answers: NDQ_002600

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answers: NDQ_002604

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answers: NDQ_002627

answers: a very large number of galaxies

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answers: It may also provide an important future constraint on dark energy

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answers: dwarf galaxies are often found near larger galaxies

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answers: galaxies are intrinsically elliptical

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answers: The gravitational lensing signal is small

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answers: galaxies are intrinsically elliptical

text: During the 1959 model year the Galaxie series was added to Ford’s full-size range and the Skyliner model was absorbed into that series. Although the 1959 Galaxie was designated as a separate series, Galaxies carried both “Fairlane 500” and “Galaxie” badging, on the rear and sides respectively. It came with the standard 292CID 2-barrel 200 hp V8.

text: During the 1959 model year the

text: Galaxie

text: series was added to Ford’s full-size range and the Skyliner model was absorbed into that series. Although the 1959 Galaxie was designated as a separate series, Galaxies carried both “Fairlane 500” and “Galaxie” badging, on the rear and sides respectively. It came with the standard 292CID 2-barrel 200 hp V8.

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