Astrophysics and Space Science

, Volume 124, Issue 2, pp 389–396 | Cite as

Mass loss from Wolf-Rayet stars

  • Mahendra Singh
  • U. S. Chaubey


The observed times of minimum light derived from the photometry of the Wolf-Rayet eclipsing binary stars CQ Cep and V444 Cyg are used to estimate the mass-loss rate of the Wolf-Rayet components in several modes of mass-loss and mass-exchange.


Mass Loss Binary Star Minimum Light 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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Copyright information

© D. Reidel Publishing Company 1986

Authors and Affiliations

  • Mahendra Singh
    • 1
  • U. S. Chaubey
    • 1
  1. 1.Uttar Pradesh State ObservatoryNaini TalIndia

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