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Stability of Emission-Line Clouds in Seyfert Galaxies
Published online by Cambridge University Press: 07 August 2017
Abstract
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Otherwise acceptable kinematic and dynamic models for emission line regions may be ruled out if the line-emitting clouds are unstable. We discuss the stability of radially-moving clouds to lateral gas flows. Such flows result from internal overpressures arising from the absorption of continuum radiation.
- Type
- Part 5: Structure of the Central Object and NLR
- Information
- Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 303 - 304
- Copyright
- Copyright © Kluwer 1989
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