Temperature distribution of the accretion disk around a black hole

Details Temperature distribution of the accretion disk around a black hole Temperature distribution of the accretion disk around a black hole

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993acaps..12..297c&link_type=abstract

Chinese Astronomy and Astrophysics (ISSN 0275-1062) Transl. of Acta Astrophysica Sinica, vol. 12, no. 4, 1992, p. 297-301., vol.

Statistics

Computation

Accretion Disks, Black Holes (Astronomy), Computational Astrophysics, Temperature Distribution, Hydrodynamic Equations, Mach Number, Numerical Integration, Optical Thickness, Thermal Stability

Scientific paper

The temperature distribution of an accretion disk around a black hole is investigated in detail by numerically integrating a system of hydrodynamic equations from the sonic point. The results obtained in this paper show that the temperature drops rapidly in the inner edge of optically thick geometrically thin disk around a black hole. Also it is found that the optically thin alpha-law disk dominated by gas pressure is thermally unstable.

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