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Search references for NGC 1012. Phrases containing NGC 1012
See searches and references containing NGC 1012!NGC 1012
Lenticular galaxy in the constellation Aries
NGC 1012 is a lenticular galaxy in the Constellation Aries. It was discovered on September 11, 1784 by William Herschel, and observed again by John Herschel
NGC_1012
Spiral galaxy in the constellation Aries
extinction. The group of galaxies around NGC 972 is sometimes referred to as the "NGC 972 group," which includes NGC 1012, NGC 1056, UGC 1958, UGC 2017, UGC 2053
NGC_972
Pair of colliding spiral galaxies in the constellation Pisces
813–836. arXiv:1012.1551. Bibcode:2011MNRAS.413..813C. doi:10.1111/j.1365-2966.2010.18174.x. S2CID 15391206. "Results for object NGC 0520". NASA/IPAC
NGC_520
Galaxy in the constellation Pisces
a stellar mass of 1.5×1012 M☉. At the center of the galaxy is a supermassive black hole with a mass of 3.0×109 M☉. List of NGC objects (1–1000) "NASA/IPAC
NGC_315
Elliptical galaxy in the constellation Virgo
known as NGC 4649, is an elliptical galaxy approximately 57 million light-years away in the equatorial constellation of Virgo. Together with NGC 4647, it
Messier_60
Galaxy in the constellation Virgo
NGC 5084 to be 1.7×1012 M☉. Koribalski et al. (2004) measured the rotational speed of NGC 5084 to be 334 km/s and calculated its mass to be 1.3×1012 M☉
NGC_5084
Galaxy in the constellation Virgo
726 (2): L21, arXiv:1012.1865, Bibcode:2011ApJ...726L..21T, doi:10.1088/2041-8205/726/2/L21, S2CID 119190993. Media related to NGC 4698 at Wikimedia Commons
NGC_4698
Galaxy in the constellation Eridanus
NGC 1232, also known as the Eye of God Galaxy is an intermediate spiral galaxy about 50 million light-years away in the constellation Eridanus. It was
NGC_1232
This is a list of NGC objects 1001–2000 from the New General Catalogue (NGC). The astronomical catalogue is composed mainly of star clusters, nebulae
List of NGC objects (1001–2000)
List_of_NGC_objects_(1001–2000)
Spiral galaxy in the constellation Virgo
Galaxies: An XMM-Newton Investigation of NGC 3367 and NGC 4536", The Astrophysical Journal, 728 (1): 25, arXiv:1012.0834, Bibcode:2011ApJ...728...25M, doi:10
NGC_4536
Galaxy in the constellation Ursa Major
NGC 3184, also known as The Little Pinwheel Galaxy, is an unbarred spiral galaxy approximately 40 million light-years away in the constellation Ursa Major
NGC_3184
Dwarf spiral galaxy in the constellation Coma Berenices
NGC 4310 is a dwarf spiral galaxy with a dust lane and ring structure located about 54 million light-years away in the constellation Coma Berenices. It
NGC_4310
Group of galaxies that includes the Milky Way
Large Magellanic Cloud, Small Magellanic Cloud, M32, NGC 205, NGC 6822, NGC 185, IC 1613 and NGC 147. He also identified IC 10 as a possible part of the
Local_Group
Galaxy in the constellation Puppis
NGC 2559 is a barred spiral galaxy in the constellation Puppis. The galaxy lies about 60 million light years away from Earth based on redshift independent
NGC_2559
Galaxy in the constellation Pegasus
NGC 7241 is 2.5×1012 M☉. There is a smaller companion galaxy superimposed on the galactic disk near its center. The companion appears bluer than NGC 7241
NGC_7241
Galaxy in the constellation Canes Venatici
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
Whirlpool_Galaxy
Planetary nebula in the constellation Vulpecula
The Dumbbell Nebula (also known as the Apple Core Nebula, Messier 27, and NGC 6853) is a planetary nebula (nebulosity surrounding a white dwarf) in the
Dumbbell_Nebula
Local supercluster home to the Milky Way
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
Virgo_Supercluster
Galaxy merger remnant in the constellation Ophiuchus
NGC 6240, also known as the Starfish Galaxy, is a nearby ultraluminous infrared galaxy (ULIRG) in the constellation Ophiuchus. It was discovered by French
NGC_6240
Radio galaxy in the constellation Centaurus
Centaurus A (also known as NGC 5128 or Caldwell 77) is a galaxy in the constellation of Centaurus. It was discovered in 1826 by Scottish astronomer James
Centaurus_A
Galaxy in the constellation Ursa Major
The Pinwheel Galaxy (also known as Messier 101, M101 or NGC 5457) is a face-on, counterclockwise intermediate spiral galaxy located 21 million light-years
Pinwheel_Galaxy
Spiral galaxy in the constellation Perseus
40 M☉·yr−1. It has a virial mass of 3×1012 M☉ and a mass-to-light ratio of 0.7. One supernova has been observed in NGC 1003: SN 1937D (Type Ia, mag. 10.5)
NGC_1003
Galaxy in the constellation Cetus
Messier 77 (M77), also known as NGC 1068 or the Squid Galaxy, is a barred spiral galaxy in the constellation Cetus. It is 35 million light-years (11 Mpc)
Messier_77
Galaxy in the constellation of Andromeda
813–836. arXiv:1012.1551. Bibcode:2011MNRAS.413..813C. doi:10.1111/j.1365-2966.2010.18174.x. S2CID 15391206. "Search specification: NGC 620". HyperLeda
NGC_620
Galaxy in the constellation Aries
NGC 770 is an elliptical galaxy in the constellation Aries. It is around 120 million light years from the Milky Way and has a diameter of around 36,000 ly
NGC_770
Galaxy in the constellation Canes Venatici
813–836. arXiv:1012.1551. Bibcode:2011MNRAS.413..813C. doi:10.1111/j.1365-2966.2010.18174.x. S2CID 15391206. "Search specification: NGC 5198". HyperLeda
NGC_5198
Open cluster in the constellation Centaurus
analysis of the open cluster NGC 5460". Monthly Notices of the Royal Astronomical Society. 413 (2): 1132–1144. arXiv:1012.3050. Bibcode:2011MNRAS.413.1132F
NGC_5460
Lenticular galaxy in the constellation Leo
813–836. arXiv:1012.1551. Bibcode:2011MNRAS.413..813C. doi:10.1111/j.1365-2966.2010.18174.x. S2CID 15391206. "Results for object NGC 3301 (NGC 3301)". NASA/IPAC
NGC_3301
Galaxy in the constellation Cetus
NGC 720 is an elliptical galaxy located in the constellation Cetus. It is located at a distance of about 80 million light years from Earth, which, given
NGC_720
Galaxy in the constellation Cancer
NGC 2775, also known as Caldwell 48, is a spiral galaxy in the constellation Cancer. It is 67 million light-years (20.5 megaparsecs) away from the Milky
NGC_2775
Globular cluster in constellation Lepus
Messier 79 (also known as M79 or NGC 1904) is a globular cluster in the southern constellation Lepus. It was discovered by Pierre Méchain in 1780 and
Messier_79
Group galaxies M31 and M32, and a few galaxies beyond the Local Group, e.g. NGC 4395. In these galaxies, the mean square (or root mean square) speed of the
List of most massive black holes
List_of_most_massive_black_holes
Galaxy in the constellation Cetus
NGC 1015 is a barred spiral galaxy, at a distance of 118 million light years in the constellation of Cetus (The Whale). It was discovered by German astronomer
NGC_1015
Galaxy in the constellation Hercules
NGC 6207 is a spiral galaxy located in the constellation Hercules. It is designated as SA(s)c in the galaxy morphological classification scheme and was
NGC_6207
Galaxy cluster in constellation Coma Berenices
3247, IC 3571 MCG 5-29- 66, NGC 4080, NGC 4150, NGC 4308, NGC 4455, NGC 4509, NGC 4534, NGC 4627, NGC 4631, NGC 4656, NGC 4670, UGC 6900, UGC 7007, UGC
Coma_I
Galaxy in the constellation of Ophiucus
NGC 6384 is an intermediate barred spiral galaxy located about 77 million light-years away in the northern part of the constellation Ophiuchus. It was
NGC_6384
Galaxy in the constellation Virgo
Messier 87 (also known as Virgo A or NGC 4486, generally abbreviated to M87) is a supergiant elliptical galaxy in the constellation Virgo that contains
Messier_87
Galaxy in the constellation Virgo
NGC 4636 is an elliptical galaxy located in the constellation Virgo. It is a member of the NGC 4753 Group of galaxies, which is a member of the Virgo II
NGC_4636
Barred spiral galaxy in the Local Group
originally named the Andromeda Nebula and is cataloged as Messier 31, M31, and NGC 224. Andromeda has a D25 isophotal diameter of about 46.56 kiloparsecs (152
Andromeda_Galaxy
diameters. The unit of measurement used is the light-year (approximately 9.46×1012 kilometers). Galaxies are vast collections of stars, planets, nebulae and
List_of_largest_galaxies
Galaxy in the constellation Antlia
mass estimate of 2.7×1012 M☉ within a radius of around 47 kpc from the galactic center. One supernova has been observed in NGC 3258. The type Ia supernova
NGC_3258
Elliptical galaxy in the constellation Virgo
NGC 4325 is an elliptical galaxy located about 330 million light-years away in the constellation Virgo. It was discovered by astronomer Heinrich d'Arrest
NGC_4325
Edge-on spiral galaxy in the constellation Virgo
NGC 5170 is a large, nearby, edge-on spiral galaxy in the equatorial constellation of Virgo. It was discovered on February 7, 1785 by William Herschel
NGC_5170
Spiral galaxy in the constellation Indus
transient ultraluminous X-ray source in NGC 7090". Monthly Notices of the Royal Astronomical Society. 501 (1): 1002–1012. arXiv:2011.08870. Bibcode:2021MNRAS
NGC_7090
Diffuse nebula in the constellation Perseus
NGC 1579 (also known as the Northern Trifid) is a diffuse nebula located in the constellation of Perseus. It is referred to as the Northern Trifid because
NGC_1579
Galaxy in the constellation Eridanus
(May 2013), "The NGC 1614 interacting galaxy. Molecular gas feeding a "ring of fire"", Astronomy & Astrophysics, 553: 11, arXiv:1303.1012, Bibcode:2013A&A
NGC_1614
Constellation straddling the celestial equator
(2021). "Isochrone fitting of Galactic globular clusters – III. NGC 288, NGC 362, and NGC 6218 (M12)". Monthly Notices of the Royal Astronomical Society
Ophiuchus
Galaxy undergoing an exceptionally high rate of star formation
close encounter with another galaxy. Starburst galaxies include M82, NGC 4038/NGC 4039 (the Antennae Galaxies), and IC 10. Starburst galaxies are defined
Starburst_galaxy
Face-on spiral galaxy in the constellation Pisces
Messier 74 (also known as NGC 628 and Phantom Galaxy) is a large spiral galaxy in the equatorial constellation Pisces. It is about 32 million light-years
Messier_74
Lenticular galaxy in the constellation Eridanus
arXiv:1012.1551. Bibcode:2011MNRAS.413..813C. doi:10.1111/j.1365-2966.2010.18174.x. S2CID 15391206. Frommert, Hartmut. "Revised NGC Data for NGC 1222"
NGC_1222
Globular cluster in the constellation Dorado
Society. 413 (2): 837–851. arXiv:1012.1476. Bibcode:2011MNRAS.413..837M. doi:10.1111/j.1365-2966.2010.18167.x. "NGC 1866". SIMBAD. Centre de données astronomiques
NGC_1866
Spiral galaxy in the constellation Leo
Galaxies: Anxmm-Newtoninvestigation of NGC 3367 and NGC 4536". The Astrophysical Journal. 728 (1): 25. arXiv:1012.0834. Bibcode:2011ApJ...728...25M. doi:10
NGC_3367
Compact astronomical body
thousands of solar masses. Primordial black holes with masses less than 1012 kg would have evaporated by now due to Hawking radiation. Despite the early
Black_hole
Seyfert galaxy in the constellation Boötes
NGC 5929 is a well-studied Seyfert galaxy in the constellation Boötes. It was discovered by English astronomer John Herschel on May 13, 1828. In the revised
NGC_5929
Galaxy in the constellation Eridanus
NGC 1600 is an elliptical galaxy in the constellation Eridanus, 149 Mly (46 Mpc) away from Earth. Often described as being an isolated early-type galaxy
NGC_1600
Unbarred lenticular galaxy in the constellation Ursa Major
NGC 3619 is an unbarred lenticular galaxy located in the northern constellation of Ursa Major. It was discovered by the German-British astronomer William
NGC_3619
Galaxy in the constellation Fornax
mass of the dark matter halo surrounding the galaxy is around 4.3 × 1012 M☉. NGC 1427 is the brightest elliptical galaxy on the eastern side of the Fornax
NGC_1427
Galaxy in the constellation Eridanus
NGC 1266 is a lenticular galaxy in the constellation Eridanus. Although not currently starbursting, it has undergone a period of intense star formation
NGC_1266
Starburst galaxy in the constellation Boötes
NGC 5930 is a starburst galaxy in the constellation Boötes that is interacting with the nearby Seyfert galaxy NGC 5929. 5930 has a morphological classification
NGC_5930
Galaxy in the constellation Ursa Major
(March 2011). "Suzaku observation of the LINER NGC 4102". Astronomy & Astrophysics. 527: 10. arXiv:1012.3080. Bibcode:2011A&A...527A.142G. doi:10
NGC_4102
Open cluster in the constellation Vela
arXiv:1012.0149. Bibcode:2011A&A...525A..16P. doi:10.1051/0004-6361/200913789. S2CID 15373925.[dead ftp link] (To view documents see Help:FTP) NGC 3228
NGC_3228
Galaxy in the constellation Andromeda
NGC 531 is a barred spiral galaxy in the constellation Andromeda with a visual magnitude of 10.51. It is a distance of 65.7 Mpc from the Sun. It is a
NGC_531
Dwarf galaxy in the constellation Eridanus with a rectangular shape
74886 has a mass of around 109 M☉ (Compared to the Milky Way's mass of about 1012 M☉). LEDA 74886 is located in the celestial sphere at a right ascension (
LEDA_74886
Aspect of physical cosmology
long wavelengths and low energies. Stars are expected to form normally for 1012 to 1014 (1–100 trillion) years, but eventually the supply of gas needed for
Future of an expanding universe
Future_of_an_expanding_universe
Open cluster
NGC 6800". "NGC 6800". "NGC Objects: NGC 6800 - 6849". Ananjevskaja, Yu.K.; Frolov, V.N.; Polyakov, E.V. "Investigation of the open star cluster NGC 6800"
NGC_6800
NGC 1313". ESO. 23 November 2006. "Trekkie Galaxy (NGC 1701) | Deep⋆Sky Corner". www.deepskycorner.ch. Retrieved 26 September 2026. "NGC 2683". NGC Online
List_of_galaxies
Binary star system in the globular cluster of Messier 4
800 parsecs (12,400 light-years) in the globular cluster of Messier 4 (M4, NGC 6121) in the constellation of Scorpius. The system is composed of a pulsar
PSR_B1620−26
Group of stars
indicates Messier 25 may constitute a ternary star cluster together with NGC 6716 and Collinder 394. Establishing precise distances to open clusters enables
Star_cluster
Postulated future astronomical event
to 5 billion years. While the Andromeda Galaxy contains about 1 trillion (1012) stars and the Milky Way about 300 billion (3×1011), the chance of even two
Andromeda–Milky_Way_collision
System of stars and interstellar matter
with numbers from certain catalogues, such as the Messier catalogue, the NGC (New General Catalogue), the IC (Index Catalogue), the CGCG (Catalogue of
Galaxy
Galaxy with a high luminosity
luminosity is 100 billion times that of the Sun. Galaxies with luminosities above 1012 L☉ are known as ultraluminous infrared galaxies (ULIRGs). Galaxies exceeding
Luminous_infrared_galaxy
Galaxy in the constellation Triangulum
NGC 740 is a barred spiral galaxy located in the Triangulum constellation. It is estimated to be 210 million light-years from the Milky Way and has a
NGC_740
Galaxy in the constellation Coma Berenices
NGC 4293 is a lenticular galaxy in the northern constellation of Coma Berenices. It was discovered by English astronomer William Herschel on March 14
NGC_4293
German currency from 1914 to 1923
1924. When it did, it replaced the Papiermark at the rate of 1-trillion (1012)-ℳ︁ to RM1. On 30 August 1924 the Rentenmark was replaced by the Reichsmark
Papiermark
Spiral galaxy in the constellation Coma Berenices
Hubble Space Telescope List of largest galaxies NGC 262, spiral galaxy surrounded by a huge H I cloud NGC 6872, large interacting barred spiral galaxy claimed
Malin_1
Spiral-shaped regions of enhanced brightness within the galactic disc in spiral galaxies
Spiral galaxies of different morphological types in the SDSS NGC 4314 (SBa) M95 (SBb) NGC 3367 (SBc) The spiral structure of galaxies exhibits considerable
Spiral_arm
Galaxy filament in the constellations Pavo, Indus and Telescopium
later be known as the NGC 134 Group, group G45 (Pavo-Indus) which would later be known as the NGC 7079, NGC 7144, NGC 7196 and NGC 7213 groups, and group
Telescopium−Grus_Cloud
Collection of more than 1,500 galaxies
Monthly Notices of the Royal Astronomical Society. 413 (2): 1236–1243. arXiv:1012.3771. Bibcode:2011MNRAS.413.1236B. doi:10.1111/j.1365-2966.2011.18210.x.
Local_Volume
Spherical collection of stars
John Herschel. The French astronomer Abbé Lacaille listed NGC 104, NGC 4833, M55, M69, and NGC 6397 in his 1751–1752 catalogue. The low resolution of early
Globular_cluster
Multiple star system in the constellation Orion
brightest member of the asterism known as Orion's Sword. It is a member of the NGC 1980 open cluster. From parallax measurements, it is located at a distance
Iota_Orionis
Zodiac constellation straddling the celestial equator
of the M74 Group. NGC 488 is an isolated face-on prototypical spiral galaxy. Two supernovae have been observed in the galaxy. NGC 520 is a pair of colliding
Pisces_(constellation)
History and future of the universe
time.[citation needed] Quantum chromodynamics phase transition 10−5 s 1012 1012 K (150 MeV/kB) The quark–gluon plasma of matter particles coalesce into
Chronology_of_the_universe
International collaboration to improve calibration of the extragalactic distance scale
The sample of galaxies include NGC 6822, IC 1613 and NGC 3109 in the Local Group, and NGC 55, NGC 247, NGC 300 and NGC 7793 in the Sculptor Group. The
Araucaria_Project
Stars sorted by absolute magnitude
massive stars: stellar parameters and rotational velocities in NGC 3293, NGC 4755 and NGC 6611". Astronomy & Astrophysics. 457 (1): 265–280. arXiv:astro-ph/0606409
List_of_most_luminous_stars
to Gliese 569". Astrophysical Journal Letters. 330 (3): L119–L123. arXiv:1012.4421. Bibcode:2011MNRAS.413.1524F. doi:10.1111/j.1365-2966.2011.18226.x.
List_of_brown_dwarfs
Relative directions of orbit or rotation
direction relative to the Milky Way's rotation, is colliding with the Milky Way. NGC 7331 is an example of a galaxy that has a bulge that is rotating in the opposite
Retrograde and prograde motion
Retrograde_and_prograde_motion
2005 supernova event in the constellation Reticulum
SN 2005df was a Type Ia supernova in the barred spiral galaxy NGC 1559, which is located in the southern constellation of Reticulum. The event was discovered
SN_2005df
Active galactic nucleus (AGN) containing a supermassive black hole
as the Sun. This quasar's luminosity is, therefore, about 4 trillion (4×1012) times that of the Sun, or about 100 times that of the total light of giant
Quasar
Peripheral nebular regions of the Orion Molecular Cloud Complex
three of these are T Tauri stars, coinciding with IRAS or X-ray sources. NGC 1788 is a small reflection nebula located about 6° west of the densest regions
Peripheral nebular regions of the Orion Complex
Peripheral_nebular_regions_of_the_Orion_Complex
Calendar year
nobleman (b. c.992) September 15 – García Sánchez III, king of Pamplona (b. c.1012) September 24 – Hermann of Reichenau, German music theorist (b. 1013) Abu
1054
Exoplanet orbiting Kepler-16
convention used for multiple star systems and extrasolar planets". arXiv:1012.0707 [astro-ph.SR]. "Kepler-16b". SIMBAD. Centre de données astronomiques
Kepler-16b
Theoretical cosmological structure
Freeman noticed that the expected decline in velocity was not present in NGC 300 nor M33, and considered an undetected mass to explain it. The DM Hypothesis
Dark_matter_halo
Astrophysical phenomenon
two further supernovae, SN 1895A and SN 1895B, were discovered in NGC 4424 and NGC 5253 respectively. Early work on what was originally believed to be
Supernova
Star in the constellation Sextans
(Santamasa) HD 92788 b KELT-11b TOI-561 b WASP-43b (Astrolábos) Galaxies NGC 2967 2974 2980 3007 3015 3018 3044 3062 3110 3115 3117 3156 3166 3169 3326
Alpha_Sextantis
our galaxy, contains about 1012 stars. Biology – Bacteria on the human body: The surface of the human body houses roughly 1012 bacteria. Computing: 1,099
Orders_of_magnitude_(numbers)
Star in the constellation Sextans
(Santamasa) HD 92788 b KELT-11b TOI-561 b WASP-43b (Astrolábos) Galaxies NGC 2967 2974 2980 3007 3015 3018 3044 3062 3110 3115 3117 3156 3166 3169 3326
Epsilon_Sextantis
Comparison of a wide range of volumes
Yervant (1999). "Hubble Space Telescope Measurements of the Expansion of NGC 6543: Parallax Distance and Nebular Evolution". Astronomical Journal. 118
Orders_of_magnitude_(volume)
American astrophysicist
extreme blue horizontal branch population in metal rich globular clusters (NGC 6388 and 6441). Rich also discovered the first known case of a luminous red
R._Michael_Rich
Radio galaxy in the constellation Draco
+72.26 is found to have a pre-existing stellar population that comprises ~1012 Msolar of stellar mass, with further ~2 per cent contributed by the current
4C_+72.26
Star in the constellation Sextans
(Santamasa) HD 92788 b KELT-11b TOI-561 b WASP-43b (Astrolábos) Galaxies NGC 2967 2974 2980 3007 3015 3018 3044 3062 3110 3115 3117 3156 3166 3169 3326
Beta_Sextantis
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NGC 1012
NGC 1012
NGC 1012
NGC 1012
NGC 1012
NGC 1012
NGC 1012
NGC 1012
NGC 1012
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