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Line and Continuum Emission from the Outer Regions of a Self-Gravitating, Magnetized Accretion Disk1

Published online by Cambridge University Press:  12 April 2016

Ye Lu ,
Lantian Yang  and
Shaoping Wu
Ye Lu
Affiliation:
Institute of Astrophysics, Huazhong Normal University, Wuhan 430070, China
Lantian Yang
Affiliation:
Institute of Astrophysics, Huazhong Normal University, Wuhan 430070, China
Shaoping Wu
Affiliation:
Institute of Astrophysics, Huazhong Normal University, Wuhan 430070, China

Abstract

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We determine the variation with radius of the physical parameters (scale height, central density, and central temperature) of a stationary self-gravitating, magnetized accretion disk at radii larger than 102RG. Our results are relevant in the context of line and continuum emission from the outer region of the disk. We have also studied the influence of self-gravitation and magnetic fields over typical radii, and have shown that the value of RBB is larger than that computed by Collin- Souffrin & Dumont by a factor of about 4.7.

Type
I. X-Rays and the Nuclear Regions of Active Galaxies
Information
International Astronomical Union Colloquium , Volume 159: Emission Lines in Active Galaxies: New Methods and Techniques , 1997 , pp. 66 - 69
Copyright
Copyright © Astronomical Society of the Pacific 1997

Footnotes

1

This work is supported by the National Natural Science Foundation of China.

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