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Astrophysics and Space Science

, Volume 73, Issue 2, pp 503–506 | Cite as

Evolution in semi-detached binary systems

  • U. S. Chaubey
Letter to the Editor

Abstract

The evolutionary process of semi-detached binary systems is examined on the basis of non-conservation of orbital angular momentum. We conclude that the semi-detached binary systems follow Type B evolution.

Keywords

Angular Momentum Evolutionary Process Binary System Orbital Angular Momentum 
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. Chaubey, U. S.: 1979,Astrophys. Space Sci. 64, 177.Google Scholar
  2. Kippenhahn, R. and Weigert, A.: 1967,Z. Astrophys. 65, 251.Google Scholar
  3. Kreiner, J. M. and Ziolkowski, J.: 1978,Acta Astron. 28, 497.Google Scholar
  4. Ziolkowski, J.: 1968, in M. Hack (ed.), ‘Mass Loss From Stars’,IAU Coll. 7, 231.Google Scholar
  5. Ziolkowski, J.: 1976, in P. Eggleton, S. Mitton, and J. Whelan (eds), ‘The Structure and Evolution of Close Binary Systems’,IAU Symp. 73, 321.Google Scholar

Copyright information

© D. Reidel Publishing Co 1980

Authors and Affiliations

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

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