Galaxy in the constellation Virgo
NGC 4318 is a smalllenticular galaxy [ 3] located about 72 millionlight-years away[ 5] in the constellationVirgo . It was discovered by astronomerJohn Herschel on January 18, 1828.[ 6] NGC 4318 is a member of theVirgo W′ group ,[ 2] [ 7] [ 8] [ 9] a group of galaxies in the background of theVirgo Cluster [ 2] that is centered on the giantelliptical galaxy NGC 4365 .[ 9]
Physical characteristics [ edit ] NGC 4318 contains a small,[ 3] classicalbulge [ 10] and a nuclear stellar disc with a diameter of ~230 ly (70 pc ).[ 11] Outside the nuclear stellar disc lies a sharply bounded, low surface brightness region with a diameter of ~1,800 ly (560 pc ) beyond which lies a larger outer disk.[ 3] [ 12]
NGC 4318 harbors asupermassive black hole with an estimated mass of 4 million ( 5× 106 M☉ )solar masses .[ 13] [ 14] [ 15]
NGC 4318 is surrounded by 18globular clusters .[ 16] [ 17]
^a b c d e f g h i "NASA/IPAC Extragalactic Database" .Results for NGC 4318 . Retrieved2019-08-31 .^a b c Merritt, David; Anthony, Andre; Peng, Eric; Jordan, Andres; Ferrarese, Laura; West, Michael; Tonry, John; Cote, Patrick; Blakeslee, John (2007-02-20). "The ACS Virgo Cluster Survey. XIII. SBF Distance Catalog and the Three-Dimensional Structure of the Virgo Cluster".The Astrophysical Journal .655 (1):144– 162.arXiv :astro-ph/0702510 .Bibcode :2007ApJ...655..144M .doi :10.1086/509598 .S2CID 16483538 . ^a b c d Bender, Ralf; Cornell, Mark E.; Fisher, David B.; Kormendy, John (2009). "Structure and Formation of Elliptical and Spheroidal Galaxies".The Astrophysical Journal Supplement Series .182 (1):216– 309.arXiv :0810.1681 .Bibcode :2009ApJS..182..216K .doi :10.1088/0067-0049/182/1/216 .S2CID 119273143 . ^ Couch, Warrick J.; Forbes, Duncan A.; Hau, George K. T.; Spolaor, Max (2010-07-05)."Early-type galaxies at large galactocentric radii - I. Stellar kinematics and photometric properties" .Monthly Notices of the Royal Astronomical Society .408 (1):254– 271.arXiv :1007.0599v1 .Bibcode :2010MNRAS.408..254S .doi :10.1111/j.1365-2966.2010.17282.x . ^ "Your NED Search Results" .ned.ipac.caltech.edu . Retrieved2019-09-01 .^ "New General Catalog Objects: NGC 4300 - 4349" .cseligman.com . Retrieved2019-08-19 .^ West, Michael J.; Tonry, John L.; Peng, Eric W.; Infante, Leopoldo; Ferrarese, Laura; Cote, Patrick; Mei, Simona; Jordan, Andres; Blakeslee, John P. (2009-01-08). "The ACS Fornax Cluster Survey. V. Measurement and Recalibration of Surface Brightness Fluctuations and a Precise Value of the Fornax--Virgo Relative Distance".The Astrophysical Journal .694 (1):556– 572.arXiv :0901.1138 .Bibcode :2009ApJ...694..556B .doi :10.1088/0004-637X/694/1/556 .S2CID 16521293 . ^ West, Michael J.; Tonry, John L.; Infante, Leopoldo; Mei, Simona; Kissler-Patig, Markus; Ferrarese, Laura; Cote, Patrick; Blakeslee, John P.; Peng, Eric W. (2010-04-16)."The ACS Fornax Cluster Survey. VIII. The Luminosity Function of Globular Clusters in Virgo and Fornax Early-Type Galaxies and its Use as a Distance Indicator" .The Astrophysical Journal .717 (2):603– 616.arXiv :1004.2883v1 .Bibcode :2010ApJ...717..603V .doi :10.1088/0004-637X/717/2/603 . ^a b Schindler, Sabine ; Vikhlinin, Alexey; Nulsen, Paul E. J.; Li, Zhiyuan; Churazov, Eugene; Zhuravleva, Irina; Zhang, Zhongli; Randall, Scott W.; Blom, Christina (2012-03-07)."Chandra observations of NGC4342, an optically faint, X-ray gas-rich early-type galaxy" .The Astrophysical Journal .755 (1): 25.arXiv :1203.1642v2 .Bibcode :2012ApJ...755...25B .doi :10.1088/0004-637X/755/1/25 .^ Romanowsky, Aaron J.; Fall, S. Michael (2018-08-07)."Angular Momentum and Galaxy Formation Revisited: Scaling Relations for Disks and Bulges" .The Astrophysical Journal .868 (2): 133.arXiv :1808.02525v2 .Bibcode :2018ApJ...868..133F .doi :10.3847/1538-4357/aaeb27 .S2CID 119061427 . ^ Ledo, H. R.; Sarzi, M.; Dotti, M.; Khochfar, S.; Morelli, L. (2010-09-01)."A census of nuclear stellar discs in early-type galaxies" .Monthly Notices of the Royal Astronomical Society .407 (2):969– 985.Bibcode :2010MNRAS.407..969L .doi :10.1111/j.1365-2966.2010.16990.x .hdl :2299/5422 .ISSN 0035-8711 . ^ West, Michael J.; Tonry, John L.; Milosavljevic, Milos; Merritt, David; Mei, Simona; Piatek, Slawomir; Blakeslee, John P.; Peng, Eric W.; Jordan, Andres (2006-02-14). "The ACS Virgo Cluster Survey. VI. Isophotal Analysis and the Structure of Early-Type Galaxies".The Astrophysical Journal Supplement Series .164 (2):334– 434.arXiv :astro-ph/0602297 .Bibcode :2006ApJS..164..334F .doi :10.1086/501350 .S2CID 18618068 . ^ Gallo, Elena; Treu, Tommaso; Marshall, Philip J.; Woo, Jong-Hak; Leipski, Christian; Antonucci, Robert (2010-05-01). "AMUSE-Virgo. II. Down-sizing in Black Hole Accretion".The Astrophysical Journal .714 (1):25– 36.arXiv :1002.3619 .Bibcode :2010ApJ...714...25G .doi :10.1088/0004-637X/714/1/25 .hdl :1721.1/95905 .ISSN 0004-637X .S2CID 53603460 . ^ Antonucci, Robert; Miller, Brendan P.; Woo, Jong-Hak; Treu, Tommaso; Gallo, Elena; Leipski, Christian (2011-11-29). "AMUSE-VIRGO. III: mid-infrared photometry of early-type galaxies and limits on obscured nuclear emission".The Astrophysical Journal .744 (2): 152.arXiv :1111.6774 .doi :10.1088/0004-637X/744/2/152 .S2CID 119203992 . ^ "VizieR" .vizier.u-strasbg.fr . Retrieved2019-09-01 .^ Alessi, Matthew; Harris, Gretchen L. H.; Harris, William E. (2013-06-10)."A Catalog of Globular Cluster Systems: What Determines the Size of a Galaxy's Globular Cluster Population?" .The Astrophysical Journal .772 (2): 82.arXiv :1306.2247v1 .Bibcode :2013ApJ...772...82H .doi :10.1088/0004-637X/772/2/82 . ^ West, Andrew A.; Tonry, John L.; Mei, Simona; Ferrarese, Laura; Chen, Chin-Wei; Blakeslee, John P.; West, Michael J.; Takamiya, Marianne; Cote, Patrick (2008-03-04)."The ACS Virgo Cluster Survey XV. The Formation Efficiencies of Globular Clusters in Early-Type Galaxies: The Effects of Mass and Environment" .The Astrophysical Journal .681 (1): 197.arXiv :0803.0330v1 .Bibcode :2008ApJ...681..197P .doi :10.1086/587951 . Wikimedia Commons has media related to
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