The Effect of a Dissipative Corona on the Structure and Stability of Cold Optically Thick Accretion Disks at High Accretion Rates
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/573/i=2/a=764/pdf
Reference22 articles.
1. The Evolution of Accretion Disks with Coronae: A Model for the Low-Frequency Quasi-periodic Oscillations in X-Ray Binaries
2. A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution
3. Cold Accretion Disks with Coronae and Advection
4. Advection‐Dominated Accretion and the Spectral States of Black Hole X‐Ray Binaries: Application to Nova Muscae 1991
5. X-ray spectra from two-phase accretion disks
Cited by 3 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
1. Gravitational instability of discs with dissipative coronae around supermassive black holes;Monthly Notices of the Royal Astronomical Society;2007-06-01
2. Accreting corona model of the X-ray variability in soft state X-ray binaries and active galactic nuclei;Astronomy & Astrophysics;2007-04-24
3. Universal spectral shape of high accretion rate AGN;Astronomy & Astrophysics;2003-11-28
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