Accretion onto a moving black hole - an exact solution

Details Accretion onto a moving black hole - an exact solution Accretion onto a moving black hole - an exact solution

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phrvl..60.1781p&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 60, May 2, 1988, p. 1781-1784.

Astronomy and Astrophysics

Astronomy

21

Accretion Disks, Binary Stars, Black Holes (Astronomy), Newtonian Fluids, Schwarzschild Metric

Scientific paper

An analytic solution for the steady-state, subsonic accretion of a gaseous medium onto a Schwarzschild or Kerr black hole is presented. The black hole moves at a constant velocity through the medium, which is uniform and at rest far from the hole and obeys a P = rho adiabatic equation of state. In the case of a rotating Kerr black hole, the flow is fully three-dimensional, but the accretion rate does not depend on the orientation of the hole's spin with respect to the incident direction of the flow.

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