A star cluster around a massive black hole - A steady-state numerical solution

Details A star cluster around a massive black hole - A steady-state numerical solution A star cluster around a massive black hole - A steady-state numerical solution

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..150b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Mar. 1980, p. 150-155.) Soviet Astronomy Letters, vol. 6, Mar.-Apr. 1980, p. 82-85.

Astronomy and Astrophysics

Astronomy

1

Black Holes (Astronomy), Star Clusters, Star Distribution, Computerized Simulation, Distribution Functions, Steady State, Stellar Envelopes

Scientific paper

An analysis is made of the structure of a star cluster surrounding a massive black hole whose mass exceeds that of the whole cluster. The stellar density distribution around the black hole and other characteristics depend significantly on the parameters of the distribution function for stars at the outer radius, which is taken equal to 20 capture radii.

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