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Evolutionary computations for intermediate mass close binary systems
Published online by Cambridge University Press: 12 April 2016
Abstract
Numerical simulations of the evolution of close binaries with primary mass between 3 and 15 Mʘ 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.
- Type
- Session VIII - Effects of Mass Loss on the Evolution of Binary Stars
- Information
- International Astronomical Union Colloquium , Volume 59: Effects of Mass Loss on Stellar Evolution , 1981 , pp. 503 - 506
- Copyright
- Copyright © Reidel 1981