Self-irradiated accretion disks around Schwarzschild black holes

Details Self-irradiated accretion disks around Schwarzschild black holes Self-irradiated accretion disks around Schwarzschild black holes

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pasj...45..443s&link_type=abstract

PASJ: Publications of the Astronomical Society of Japan (ISSN 0004-6264), vol. 45, no. 3, p. 443-448.

Statistics

Computation

9

Accretion Disks, Black Holes (Astronomy), Gravitational Effects, Relativistic Effects, Schwarzschild Metric, Active Galactic Nuclei, Computational Astrophysics, Luminosity, Ray Tracing, Viscosity

Scientific paper

A full relativistic numerical simulation is used to recalculate the self-irradiated luminosity L(o) of the disk as a function of the inclination angle for the case of the Schwarzschild black hole (SBH). It is found that the ratio of L(o) to the canonical disk luminosity L(d) i.e., the face-on disk luminosity without self-irradiation) is 0.18 when the disk is edge-on. The structure and spectrum of self-irradiated accretion disks around a SBH are obtained for the cases of X-ray binaries and active galactic nuclei.

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