The Transition from an Optically Thick Disk to an Optically Thin Disk

Details The Transition from an Optically Thick Disk to an Optically Thin Disk The Transition from an Optically Thick Disk to an Optically Thin Disk

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999bha..proge..35m&link_type=abstract

Presented at the KITP Program: Black Hole Astrophysics, May 18, 1999, Kavli Institute for Theoretical Physics, University of Cal

Astronomy and Astrophysics

Astrophysics

Scientific paper

with Dr. Shoji Kato (ITP & Kyoto Univ)I discuss the transition from an optically thick cool Shakura-Sunyaev disk to anoptically thin hot advection-dominated accretion flow at certain radius whichmight give explanations to the low state spectra of black hole X-ray binaries.The main point in our model is the inclusion of the turbulent energy transport(the turbulent condution). By solving the 1D rad-hydro equation we obtain theseries of global solutions with transiti

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