Hostname: page-component-788cddb947-w95db Total loading time: 0 Render date: 2024-10-19T05:22:33.431Z Has data issue: false hasContentIssue false

Correlation between flare stars and other populations in young clusters and star forming regions

Published online by Cambridge University Press:  23 September 2016

V. S. Shevchenko
Affiliation:
Astronomical Institut Uzbek Academy of Sciences USSR
S. D. Yakubov
Affiliation:
Astronomical Institut Uzbek Academy of Sciences USSR

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.

Ratio between number OB-stars and that of comparatively bright flare stars in star forming reions are discussed.

Type
III Flare Stars and Related Objects Fuors and Other Non-Stable Objects
Copyright
Copyright © Kluwer 1990 

References

Shevchenko, V.S. (1979), Astronomicheski Jurnal 57, p.1162.Google Scholar
Shevchenko, V.S. (1989), Ae/Be Herbig Stars, FAN, Tashkent, Stalbovski, O.I., and Shevchenko, V.S. (1980), Flare stars, fuors, and Herbig-Haro objects, ed. Mirzoyan, L.V., Academy Sci. Arm SSR, Yerevan, p.116.Google Scholar