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Gaseous response to bar-like distortions

Published online by Cambridge University Press:  14 August 2015

William W. Roberts Jr.
William W. Roberts Jr.*
Affiliation:
University of Virginia

Extract

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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 

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