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high-energy astrophysics > black hole > supermassive black hole

Terme préférentiel

supermassive black hole  

Définition(s)

  • A supermassive black hole (SMBH or sometimes SBH) is the largest type of black hole, with its mass being on the order of hundreds of thousands, or millions to billions of times the mass of the Sun (M☉). Black holes are a class of astronomical objects that have undergone gravitational collapse, leaving behind spheroidal regions of space from which nothing can escape, not even light. Observational evidence indicates that almost every large galaxy has a supermassive black hole at its center. For example, the Milky Way has a supermassive black hole in its Galactic Center, corresponding to the radio source Sagittarius A*. Accretion of interstellar gas onto supermassive black holes is the process responsible for powering active galactic nuclei (AGNs) and quasars. (Wikipedia, The Free Encyclopedia, https://en.wikipedia.org/wiki/Supermassive_black_hole)

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RDF/XML TURTLE JSON-LD Dernière modif. 24/04/2023