Spectral Properties of Accretion Disks Around Galactic and Extragalactic Black Holes

Details Spectral Properties of Accretion Disks Around Galactic and Extragalactic Black Holes Spectral Properties of Accretion Disks Around Galactic and Extragalactic Black Holes

1995-10-02

arxiv.org/abs/astro-ph/9510005v2

Astrophys.J. 455 (1995) 623

Astronomy and Astrophysics

Astrophysics

45 pages of Latex file + 10 figures (Misprints in Description and Caption of Figure 2 are corrected)

Scientific paper

10.1086/176610

We study the spectral properties of a very general class of accretion disks which can be decomposed into three distinct components apart from a shock at $r=r_s$: (1) An optically thick Keplerian disk on the equatorial plane ($r>r_s$), (2) A sub-Keplerian optically thin halo above and below this Keplerian disk $r>r_s$ and (3) A hot, optically slim, $\tau\sim 1$ postshock region $r

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