1990 Chin, C.-W., and R.B. Stothers 1990. Tables and intercomparisons of evolutionary sequences of models for massive stars. These parameters include the interior convective mixing scheme, the mixing length in the outer convective envelope, the rate of stellar-wind mass loss, the initial stellar mass, and the initial chemical composition. The tables cover evolution of the star from the zero-age main sequence to either the end of core hydrogen burning or the end of core helium burning.
M sol .
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