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Evolution of Galaxies Governed by Disk Dynamics and Spiral Structure

Published online by Cambridge University Press:  12 April 2016

Raymond J. Talbot Jr.
Raymond J. Talbot Jr.*
Affiliation:
Department of Space Physics and Astronomy, Rice University Houston, Texas 77001

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My major topic will be the evolutionary changes in disk galaxies caused by the continuing process of star formation. The task of interpreting observations to derive the past rate of star formation is treacherous, as I am sure will be evident in the various observational papers presented at this colloquium. Therefore, I will mention only briefly some of the basic aspects of models which have been used to discuss that past evolution.

Type
Part I: Formation and Evolution of Disc Galaxies
Information
International Astronomical Union Colloquium , Volume 45: Chemical and Dynamical Evolution of our Galaxy , September 1977 , pp. 31 - 45
Copyright
Copyright © Geneva Observatory 1977

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