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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De Loore, C., Vanbeveren, D. Results of evolutionary computations of primaries of close binaries with different initial composition. Space Sci Rev 66, 391–394 (1993). https://doi.org/10.1007/BF00771088
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DOI: https://doi.org/10.1007/BF00771088