Schedule May 18, 1999
The Transition from an Optically Thick Disk to an Optically Thin Disk
Dr. Tadahiro Manmoto, ITP & Kyoto Univ
with Dr. Shoji Kato (ITP & Kyoto Univ) I discuss the transition from an optically thick cool Shakura-Sunyaev disk to an optically thin hot advection-dominated accretion flow at certain radius which might 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 the series of global solutions with transiti

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