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A comparison between the orbital masses of early type binary components and masses predicted by stellar evolution

  • M. Vrancken
  • W. van Rensbergen
  • D. Vanbeveren
I. “Norman” Early-Type Stars
Part of the Lecture Notes in Physics book series (LNP, volume 401)

Abstract

In this paper we show that for eight components of early type binary systems (including three supergiants) the orbital mass corresponds reasonably well with masses resulting from evolutionary computations.

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References

  1. Hubeny, I., 1988, Comp. Phys. Comm. 52, 103.Google Scholar
  2. Joss, P.C., Rappaport, S.A., 1984, Ann. Rev. Astron. Astrophys. 22, 537.Google Scholar
  3. Kudritzki, R.P. and Hummer, D.G., 1986, in Luminous Stars and Associations in Galaxies, editors C.W.H. De Loore et al.Google Scholar
  4. Kurucz, 1991, private communication.Google Scholar
  5. Maeder, A.,1991, Astron. Astrophys. (in press).Google Scholar
  6. Popper, D.M., 1980, Ann. Rev. Astron. Astrophys. 18, 115.Google Scholar
  7. Vanbeveren, D.: 1990, Astron. Astrophys. 234, 243.Google Scholar

Copyright information

© Springer-Verlag 1992

Authors and Affiliations

  • M. Vrancken
    • 1
  • W. van Rensbergen
    • 1
  • D. Vanbeveren
    • 2
  1. 1.Astrophysical InstituteVrije Universiteit BrusselsBrussels
  2. 2.I.H. Group T LeuvenLeuven

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