Sound horizon of accretion onto a Kerr black hole |
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| Authors: | J. F. Lu |
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| Affiliation: | (1) International School for Advanced Studies, Trieste, Italy;(2) University of Science and Technology of China, Hefei, China |
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| Abstract: | ![]()
Two accretion modes (disclike and Bondi type), based on a discontinuous change in location of the sound horizon, exist generally for accretion onto a Kerr black hole, except for the case of a corotating accretion flow onto a very rapidly rotating hole, in which only Bondi-type mode is possible. |
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