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On Shock Conditions in Black-Hole Accretion1
Published online by Cambridge University Press: 12 April 2016
Abstract
We study the effects of different shock conditions upon shock properties, such as their location and strength. We find that it is very important to include the effects of radiative energy loss in the shock front.
- Type
- I. X-Rays and the Nuclear Regions of Active Galaxies
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- Copyright
- Copyright © Astronomical Society of the Pacific 1997
Footnotes
This work is supported by the National Natural Science Foundation of China.
References
1 This work is supported by the National Natural Science Foundation of China.