Abstract
The present paper summarizes fundamental evolutionary parameters of primaries of close binaries with initial masses between 9 and 60 M⊙ and initial composition appropriate for the Galaxy, the LMC and the SMC. The primary timescales and WR binary timescales are compared with corresponding recent single star predictions.
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© 1994 Springer Science+Business Media Dordrecht
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De Loore, C., Vanbeveren, D. (1994). Results of Evolutionary Computations of Primaries of Close Binaries with Different Initial Composition. In: Vanbeveren, D., van Rensbergen, W., de Loore, C. (eds) Evolution of Massive Stars. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1080-8_47
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DOI: https://doi.org/10.1007/978-94-011-1080-8_47
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-4471-4
Online ISBN: 978-94-011-1080-8
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