Hostname: page-component-6bf8c574d5-2jptb Total loading time: 0 Render date: 2025-02-23T11:16:09.048Z Has data issue: false hasContentIssue false
  • English
  • Français

Flare Stars in Evolved Clusters

Published online by Cambridge University Press:  14 August 2015

E. S. Parsamian
E. S. Parsamian*
Affiliation:
Byurakan Astrophysical Observatory, Armenia, USSR

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.

A new method of determination of the ages of aggregates based on flare star observations is proposed. The method is specially useful in the case of young clusters and associations, for which the usual method involving their H-R diagrams encounters difficulties. The method can be used also for particular flare stars.

Type
August 28 Open Clusters
Information
Symposium - International Astronomical Union , Volume 85: Star Clusters , 1980 , pp. 249 - 250
Copyright
Copyright © Reidel 1980 

References

Parsamian, E. S.: 1976, Astrofis. 12, 235.Google Scholar
Parsamian, E. S.: 1978, in Balázs, B. A. (ed.) Star Cluster Symposium, Eötvös University Press, Budapest, p. 119.Google Scholar
Ambartsumian, V. A.: 1978, Astrofis. 14, 367.Google Scholar