Hostname: page-component-77c89778f8-5wvtr Total loading time: 0 Render date: 2024-07-21T00:04:05.035Z Has data issue: false hasContentIssue false
  • English
  • Français

Young W UMa Binaries and the Interaction with their Environment

Published online by Cambridge University Press:  12 April 2016

F. Van’t Veer
F. Van’t Veer*
Affiliation:
Institut d’Astrophysique, 75014 Paris - France

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.

It is arpued that late type W UMa binaries undergo mass ejection, mainly through the second Lagragian point, which causes a steady decrease of their mass ratio m2/m1. This makes it reasonable to believe that the W UMa stage is a state of transition between T Tau and normal main sequence stars.

Type
Part II: Cataclysmic Variables
Information
International Astronomical Union Colloquium , Volume 42: The Interaction of Variable Stars with their Environment , 1977 , pp. 388 - 392
Copyright
Copyright © Veröff. Der Remeis-Sterwarte 1977

References

Binnendijk, L.: 1970, Vistas in Astronomy, 12, 217 Google Scholar
Hutchings, J.B., Hill, G.: 1973, Astrophys. J. 179, 539 Google Scholar
Mullan, D.J.: 1975, Astrophys. J., 198, 563.Google Scholar
Nariai, K.: 1976, Publ. Astr. Soc. Japan, 28, 593.Google Scholar
Nariai, K.: 1977, Private Communication Google Scholar
Van’t Veer, F.: 1975, Astron. Astrophys., 40, 167 Google Scholar
Van’t Veer, F.: 1976, Structure and Evolution of Close Binary Systems, Ed. Eggleton, P. et al, p. 343, IAU Symposium n°73.CrossRefGoogle Scholar
Worden, S.P., WHelan, J.: 1973, Mon. Not. Roy. Astr. Soc. 163, 391.Google Scholar