Liu, Mineshige, & Shibata, Magnetic Reconnection-heated Corona
1998, who claim that only the soft state is realized); (3) at low luminosity (L < 0.1LEdd) most of the accretion energy is transferred to the corona and the...
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arXiv:astro-ph/9609180 v1 26 Sep 1996
Edd. ratio and the. viscosity parameter α, the same in the disk and in the. corona. At each radius r we calculate the fraction of...
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Spectra from a Magnetic Reconnection-heated Corona in Active ...
We investigate a corona coupled with an underlying disk through the magnetic... For low-luminosity systems (L<~0.2LEdd) there exists only the solution of...
