Results of evolutionary computations of primaries of close binaries with different initial composition

Details Results of evolutionary computations of primaries of close binaries with different initial composition Results of evolutionary computations of primaries of close binaries with different initial composition

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ssrv...66..391d&link_type=abstract

Space Science Reviews, Volume 66, Issue 1-4, pp. 391-394

Computer Science

1

Stars:Stellar Evolution, Stars:Massive Binaries

Scientific paper

The present paper summarizes fundamental evolutionary parameters of
primaries of close binaries with initial masses between 9 and 60
M&sun; 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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