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The Hα Line Profile in Early Type-Binary Systems HD 47129 and γ Velorum

  • R. Rajamohan

Abstract

A brief description of the variation of the Hα Line profile in γ Velorum and HD 47129 is given.

Keywords

Velocity Curve Stellar Wind Common Centre Emission Component Double Star 
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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References

  1. Abhyankar, K. D.: 1959, Astrophys. J. Suppl. 4, 147.ADSCrossRefGoogle Scholar
  2. Batten, A. H.: 1973, Binary and Multiple Systems of Stars, Pergamon Press, p. 112.Google Scholar
  3. Hutchings, J. B.: 1976, Astrophys. J. 206, 490.ADSCrossRefGoogle Scholar
  4. Sahade, J.: 1962, in J. Sahade (ed.), Symposium on Stellar Evolution, La Plata Observatory, p. 185.Google Scholar
  5. Struve, O., Sahade, J., and Huang, S. S.: 1958, Astrophys. J. 127, 148.ADSCrossRefGoogle Scholar

Copyright information

© D. Reidel Publishing Company, Dordrecht, Holland 1984

Authors and Affiliations

  • R. Rajamohan
    • 1
  1. 1.Indian Institute of AstrophysicsBangaloreIndia

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