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Semiconvection mixing and its influence on case B mass exchange in massive binaries
E. I. Staritsin
Journal:

Symposium - International Astronomical Union / Volume 163 / 1995

Published online by Cambridge University Press:

07 August 2017, pp. 324-325

Print publication:

1995
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In case of moderate matter mixing in the semi-convective zone the primary loses part of its mass on a nuclear time-scale. It looks like a CNO-supergiant during the first part of the helium burning stage. Another part of the mass is lost on the thermal time-scale. The primary looks like a WR star during the second part of the helium burning stage.