Sound horizon of accretion onto a Kerr black hole

Details Sound horizon of accretion onto a Kerr black hole Sound horizon of accretion onto a Kerr black hole

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986gregr..18...45l&link_type=abstract

General Relativity and Gravitation (ISSN 0001-7701), vol. 18, Jan. 1986, p. 45-51.

Astronomy and Astrophysics

Astronomy

26

Accretion Disks, Black Holes (Astronomy), Kerr Effects, Stellar Mass Accretion, Corotation

Scientific paper

It is proved that two accretion modes (a disk-like mode and a Bondi-type mode) arising due to discontinuous changes in the location of the sound horizon exist generally in the case of accretion onto a Kerr black hole. The dual accretion modes do not exist in the case of flow onto a very rapidly rotating black hole, where only the Bondi-type accretion mode is possible.

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