Relativistic Super-Critical Accretion Disks

Details Relativistic Super-Critical Accretion Disks Relativistic Super-Critical Accretion Disks

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.386b&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present the results of fully relativistic calculations of the
super-critical advective disk around a Kerr black hole. Such disks may
form in quasars, the brightest AGNs. In the case of large viscosity
parameter, alpha > 0.03, the disk deviates from the black body state
and overheats up to a temperature T ~3 times 10^8 K.

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