The evolution of a massive black hole in the nucleus of a normal galaxy

Details The evolution of a massive black hole in the nucleus of a normal galaxy The evolution of a massive black hole in the nucleus of a normal galaxy

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..387d&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, May 1989, p. 387-395. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

2

Black Holes (Astronomy), Galactic Nuclei, Milky Way Galaxy, Stellar Evolution, Neutron Stars, Star Clusters, Stellar Physics

Scientific paper

At the contraction stage of a stellar system, the evolution of a stellar cluster in the nucleus of a normal galaxy with a massive black hole leads to a sudden growth in the black hole due to tidal destruction and absorption of stars. The contraction of the stellar system is followed by an expansion caused by heating due to stars that are gravitationally bound with the black hole. The growth of the black hole during this expansion stage slows down and, in the case of the Galaxy, the mass of the black hole 'freezes' at a level less than about 10 to the 6th solar masses.

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