Accretion onto a moving black hole - A fully relativistic treatment

Details Accretion onto a moving black hole - A fully relativistic treatment Accretion onto a moving black hole - A fully relativistic treatment

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...336..313p&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 336, Jan. 1, 1989, p. 313-349.

Statistics

Computation

49

Black Holes (Astronomy), Computational Astrophysics, Relativistic Effects, Stellar Mass Accretion, Adiabatic Conditions, Flow Velocity, Mach Number, Velocity Distribution

Scientific paper

The effect of constant-rate motion through a uniform adiabatic medium on the steady-state accretion of matter onto a Schwarzschild black hole is investigated theoretically by means of numerical simulations. The derivation of the model is given in detail, and the results are presented in extensive graphs. The appearance of the flows and the accretion rates are found to be in good agreement with published data for the Newtonian regime and generally similar for the relativistic case.

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