Hostname: page-component-77c89778f8-7drxs Total loading time: 0 Render date: 2024-07-17T17:25:39.332Z Has data issue: false hasContentIssue false
  • English
  • Français

A theory of galactic evolution

Published online by Cambridge University Press:  14 August 2015

S. V. M. Clube
S. V. M. Clube*
Affiliation:
Royal Observatory, Edinburgh, Scotland

Extract

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.

…“there exist many galaxies where most of the light originates in an apparently flat rotating disk, and where the random stellar motions appear to be small compared to the systematic circular motion i.e. they are apparently “cold.” Our own Galaxy is such a system, and it does not seem to suffer any large scale, large amplitude, short-time-scale instability”… Ostriker and Peebles, Ap. J. 186, 467, 1973.

Type
IV. GALACTIC KINEMATICS AND DISTANCES
Information
Symposium - International Astronomical Union , Volume 84: The Large-Scale Characteristics of the Galaxy , 1979 , pp. 239 - 241
Copyright
Copyright © Reidel 1979 

References

Clube, S. V. M.: 1978, Vistas in Astronomy 22.CrossRefGoogle Scholar
van der Kruit, P. C., Oort, J. H., and Mathewson, D. W.: 1972, Astron. Astrophys. 21, 169.Google Scholar