Abstract

Detailed calculations of the contribution of the trapped line photons to the overall pressure in line-emitting regions around active galactic nuclei are presented. They lead to the conclusion that radiation pressure is a significant factor in determining the stability of these clouds.

Document Type

Article

Publication Date

6-1-1986

Notes/Citation Information

Published in The Astrophysical Journal, v. 305, no. 1, p. 35-44.

© 1986. The American Astronomical Society. All rights reserved.

The copyright holder has granted permission for posting the article here.

Digital Object Identifier (DOI)

http://dx.doi.org/10.1086/164226

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