On the evolutionary time scale of the accreting component in massive close binaries: consequences for the supernova event

On the evolutionary time scale of the accreting component in massive close binaries: consequences for the supernova event

The remaining core hydrogen burning lifetime after a case B of mass exchange is computed for the mass gaining component in massive close binaries. Effects of stellar wind mass loss and mass loss during Roche Lobe OverFlow (RLOF) are included. Consequences for the evolutionary scenario are discussed.

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Veröffentlicht in:International Astronomical Union Colloquium 1981, Vol.59, p.465-468
Hauptverfasser: Doom, C., De Grève, J.P.
Format: Artikel
Sprache:eng
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Zusammenfassung:The remaining core hydrogen burning lifetime after a case B of mass exchange is computed for the mass gaining component in massive close binaries. Effects of stellar wind mass loss and mass loss during Roche Lobe OverFlow (RLOF) are included. Consequences for the evolutionary scenario are discussed.
ISSN:0252-9211
DOI:10.1017/S0252921100095129