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Do Galaxies Evolve Along the R – ω Sequence?

Published online by Cambridge University Press:  14 August 2015

William C. Saslaw
William C. Saslaw*
Affiliation:
Berkeley Astronomy Dept., University of California, and Institute of Theoretical Astronomy, University of Cambridge, and Center for Advanced Studies, University of Virginia

Abstract

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The stellar contents of Sb and Sc galaxies do not appear to be related to their rotation properties. This lack of correlation suggests that the position of a galaxy on the R – ω sequence is determined to a large extent by the environment in which the galaxy formed, rather than by subsequent evolution.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 44: External Galaxies and Quasi-Stellar Objects , 1972 , pp. 93 - 96
Copyright
Copyright © Reidel 1972 

References

Saslaw, W. C.: 1970, Astrophys. J. 160, 11.CrossRefGoogle Scholar
Saslaw, W. C.: 1971a, Astrophys. J. 163, 249.CrossRefGoogle Scholar
Saslaw, W. C.: 1971b, Monthly Notices Roy. Astron. Soc. 152, 341.CrossRefGoogle Scholar