Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-26T06:37:59.212Z Has data issue: false hasContentIssue false

On Shock Conditions in Black-Hole Accretion1

Published online by Cambridge University Press:  12 April 2016

Feng Yuan
Affiliation:
Center for Astrophysics, University of Science and Technology of China, Hefei, Anhui, 230026, China
Ju-Fu Lu
Affiliation:
Center for Astrophysics, University of Science and Technology of China, Hefei, Anhui, 230026, China

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Copyright
Copyright © Astronomical Society of the Pacific 1997

Footnotes

1

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.