Statistics – Computation
Scientific paper
Mar 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.189..141c&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 189, no. 1, March 1992, p. 141-145.
Statistics
Computation
Accretion Disks, Black Holes (Astronomy), Viscosity, X Ray Spectra, Astronomical Spectroscopy, Computational Astrophysics
Scientific paper
The modified alpha-viscosity law is employed with attention given to electron-scattering opacity and free-free absorption opacity to define the X-ray spectrum of a black hole's accretion disk. The equations of the disk structure are solved numerically and demonstrate that the accretion rate must be less than the limit 0.25Mcr due to the requirement for geometrically thin disks. The present treatment describes the contribution of the disk's transient regions to the X-ray spectrum and calls into question previous results that ignored the critical accretion rate.
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