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Article contents
Gaseous response to bar-like distortions
Published online by Cambridge University Press: 14 August 2015
Extract
In this review the large-scale dynamics of the gas in a model disk galaxy which has an oval, bar-like distortion (or bar structure) in the inner parts is reviewed from the standpoint of recent gas dynamical studies, both steady state and time evolutionary.
- Type
- III. SPIRAL STRUCTURE
- Information
- Symposium - International Astronomical Union , Volume 84: The Large-Scale Characteristics of the Galaxy , 1979 , pp. 175 - 186
- Copyright
- Copyright © Reidel 1979