Adiabatic growth of a black hole in a rotating stellar system

Details Adiabatic growth of a black hole in a rotating stellar system Adiabatic growth of a black hole in a rotating stellar system

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...343..594l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 343, Aug. 15, 1989, p. 594-601.

Astronomy and Astrophysics

Astronomy

29

Black Holes (Astronomy), Galactic Nuclei, Stellar Motions, Stellar Systems, Density Distribution, Distribution Functions, Poisson Equation, Stellar Rotation

Scientific paper

The consequences of slowly adding a massive black hole to the center of a rotating stellar system are considered. Although both the rotation velocity V and the velocity dispersion sigma increase when the black hole is added, the rotation velocity increases faster. The effect goes in the right direction but is too gradual to explain the V/sigma profiles recently observed in several galactic nuclei.

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