Knowledge (XXG)

Central massive object

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The most massive galaxies are thought to always contain a supermassive black hole (SBH); these galaxies do not contain nuclear star clusters, and the CMO is identified with the SBH. Fainter galaxies usually contain a nuclear star cluster (NSC). In most of these galaxies, it is not known whether a
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Nishiyama, S.; Schödel, R. (2012). "Young, Massive Star Candidates Detected throughout the Nuclear Star Cluster of the Milky Way".
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Böker, Torsten (2010b). "Young Massive Star Clusters in the Era of the Hubble Space Telescope". In Macchetto, F. Duccio (ed.).
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supermassive black hole is present, and the CMO is identified with the NSC. A few galaxies, for instance the
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Böker, Torsten (2010a). "Nuclear star clusters". In de Grijs, Richard; Lépine, Jacques R. D. (eds.).
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scientist Torsten Böker observes that some galaxies appear to have neither SBHs nor NSCs.
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Star Clusters (IAU S266): Basic Galactic Building Blocks Throughout Time and Space
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galaxies have CMOs, and that a common mechanism of galaxy formation causes both,
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The mass associated with CMOs is roughly 0.1–0.3% times the total mass of the
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The star-like nucleus at the centre of this edge-on spiral galaxy,
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You can help Knowledge (XXG) by 14: 107:Although this is suggestive that 1142: 1116: 1105: 1104: 22: 1047:Galaxy formation and evolution 1042:Galaxy color–magnitude diagram 32:, is a central massive object. 1: 205:Astronomy & Astrophysics 929:Galaxies named after people 235:10.1051/0004-6361/201219773 1246: 1137: 1062:Gravitational microlensing 1017:Galactic coordinate system 190:Princeton University Press 16:Central object of a galaxy 1100: 92:, or even both together. 37: 21: 1210:Supermassive black holes 1027:Galactic magnetic fields 840:Brightest cluster galaxy 736:Luminous infrared galaxy 1220:Stellar astronomy stubs 1022:Galactic habitable zone 1007:Extragalactic astronomy 596:Supermassive black hole 510:Active galactic nucleus 135:Core collapse (cluster) 86:supermassive black hole 1154:-related article is a 774:Low surface brightness 525:Central massive object 80:, such as a galaxy or 70:central massive object 1205:Astrophysics concepts 1052:Galaxy rotation curve 1087:Population III stars 1082:Intergalactic travel 1032:Galactic orientation 899:Voids and supervoids 90:nuclear star cluster 1077:Intergalactic stars 966:Large quasar groups 961:Groups and clusters 825:Groups and clusters 684:Lyman-alpha emitter 576:Interstellar medium 227:2012yCat..35490057N 1230:Astrophysics stubs 1072:Intergalactic dust 1057:Gravitational lens 1012:Galactic astronomy 981:Starburst galaxies 721:blue compact dwarf 677:Energetic galaxies 641:BL Lacertae object 1167: 1166: 1132: 1131: 1092:Galaxy X (galaxy) 1067:Illustris project 1037:Galactic quadrant 758:Wolf-Rayet galaxy 748:Green bean galaxy 743:Hot dust-obscured 694:Luminous infrared 458:Elliptical galaxy 188:. 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Index


NGC 4244
v
t
e
star system
globular cluster
supermassive black hole
nuclear star cluster
Milky Way
NGC 4395
ESA
MIRI
galactic bulge
Core collapse (cluster)
Galactic Center
Stellar dynamics
Böker 2010a


Merritt, David
Dynamics and Evolution of Galactic Nuclei
Princeton University Press
arXiv
1210.6125
Bibcode
2012yCat..35490057N
doi
10.1051/0004-6361/201219773
S2CID

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