Physics
Scientific paper
Jun 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011japa...32..293z&link_type=abstract
Journal of Astrophysics and Astronomy, Volume 32, Issue 1-2, pp. 293-294
Physics
Accretion, Accretion Disks, Black Hole Physics, Instabilities
Scientific paper
The standard thin disk model predicts that when the accretion rate is moderately high, the disk is radiation-pressure-dominated and thermally unstable. However, observations indicate the opposite, namely the disk is quite stable. We present an explanation in this work by taking into account the role of the magnetic field which was ignored in the previous analysis.
Gu Wei-Min
Lu Ju-Fu
Yuan Fang-Fang
Zheng Sheng-Ming
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