Hostname: page-component-84b7d79bbc-g7rbq Total loading time: 0 Render date: 2024-07-25T22:25:52.795Z Has data issue: false hasContentIssue false
  • English
  • Français

Multiple Stars as A Result of the Dynamical Evolution of Small Stellar Systems

Published online by Cambridge University Press:  12 April 2016

Avram Hayli
Avram Hayli*
Affiliation:
Université de Besançon

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.

Some double, triple or quadruple stars could be the final stage of the dynamical evolution of small galactic clusters. This evolution is nothing but a redistribution of the kinetic and mutual potential energy of the stars. It has two main effects: the escape of stars from the cluster and the formation of tight subsystems.

Type
Session 6
Information
International Astronomical Union Colloquium , Volume 33: Observational Parameters and Dynamical Evolution of Multiple Stars , May 1977 , pp. 207 - 208
Copyright
Copyright © Otto G. Franz and Paris Pismis 1977

References

Hayli, A. 1971, Ap. and Space Sci., 13, 309.Google Scholar