Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q16256303> ?p ?o }
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- Q16256303 subject Q7139523.
- Q16256303 subject Q9405142.
- Q16256303 abstract "Central massive object (CMO) refers to a mass concentration at the center of a galaxy.It can be either a supermassive black hole or a nuclear star cluster, i.e., a dense cluster of stars.The most massive galaxies are believed 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 supermassive black hole is present, and the CMO is identified with the NSC. A few galaxies, for instance the Milky Way and NGC 4395, are known to contain both a SBH and a NSC. The mass associated with CMOs is roughly 0.1-0.3% times the total mass of the galactic bulge.".
- Q16256303 thumbnail NGC4244.jpg?width=300.
- Q16256303 wikiPageWikiLink Q2488.
- Q16256303 wikiPageWikiLink Q321.
- Q16256303 wikiPageWikiLink Q40392.
- Q16256303 wikiPageWikiLink Q6333.
- Q16256303 wikiPageWikiLink Q7139523.
- Q16256303 wikiPageWikiLink Q736657.
- Q16256303 wikiPageWikiLink Q9405142.
- Q16256303 wikiPageWikiLink Q942001.
- Q16256303 comment "Central massive object (CMO) refers to a mass concentration at the center of a galaxy.It can be either a supermassive black hole or a nuclear star cluster, i.e., a dense cluster of stars.The most massive galaxies are believed to always contain a supermassive black hole (SBH); these galaxies do not contain nuclear star clusters, and the CMO is identified with the SBH.".
- Q16256303 label "Central massive object".
- Q16256303 depiction NGC4244.jpg.