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Evolutionary Computations for Intermediate Mass Close Binary Systems

  • Th. J. van der Linden
Part of the Astrophysics and Space Science Library book series (ASSL, volume 89)

Abstract

Numerical simulations of the evolution of close binaries with primary mass between 3 and 15 M and mass ratios of ∼1.5 were carried out. These results show that after mass transfer the system consists of a bright main-sequence star together with a faint He-star in a rather wide orbit (p> 60d) Evolution of this kind predicts isotope anomalies for the CNO-elements with respect to their solar values.

Keywords

Massive Star Convective Zone Close Binary Primary Mass Convective Core 
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. CAMERON in Proceedings of the conference on Explosive Nucleo Synthesis, 1973Google Scholar
  2. Kriz, S. and Harmanec P. 1975, Bull. Astron. Inst. Czech. 26, 65ADSGoogle Scholar

Copyright information

© D. Reidel Publishing Company 1981

Authors and Affiliations

  • Th. J. van der Linden
    • 1
  1. 1.Astronomical InstituteUniversity of AmsterdamThe Netherlands

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