Self‐consistent Thermal Accretion Disk Corona Models for Compact Objects. I. Properties of the Corona and the Spectrum of Escaping Radiation-Reference-Cited by-同舟云学术

Self‐consistent Thermal Accretion Disk Corona Models for Compact Objects. I. Properties of the Corona and the Spectrum of Escaping Radiation

Published:1997-10 Issue:2 Volume:487 Page:747-758
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Dove James B.,Wilms Jorn,Begelman Mitchell C.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/487/i=2/a=747/pdf

Reference62 articles.

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2. Arnaud, K. A. 1996, in ASP Conf. Ser. 101, Astronomical Data Analysis Software and Systems V, ed. G. H. Jacoby & J. Barnes (San Francisco: ASP), 17

3. A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution

4. Nonlinear Stability, Hydrodynamical Turbulence, and Transport in Disks

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