Cepheid Evolution with Pulsationally-Driven Mass Loss

We have studied the effects of a pulsationally-driven wind on Cepheid evolution. Mass loss due to the wind, which occurs only when the star is crossing the Cepheid instability strip, is a function of luminosity and radius. We have investigated the evolution of 4, 5, 6, 7 and 8 M ⊙ stars using the up...

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Veröffentlicht in:International Astronomical Union Colloquium 1989, Vol.111, p.252-252
Hauptverfasser: Brunish, Wendee M., Willson, Lee Anne
Format: Artikel
Sprache:eng
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Zusammenfassung:We have studied the effects of a pulsationally-driven wind on Cepheid evolution. Mass loss due to the wind, which occurs only when the star is crossing the Cepheid instability strip, is a function of luminosity and radius. We have investigated the evolution of 4, 5, 6, 7 and 8 M ⊙ stars using the updated 12 C(α,γ) 16 O rates.
ISSN:0252-9211
DOI:10.1017/S025292110001160X