Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-25T15:20:39.867Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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