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 |
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Hauptverfasser: | , |
Format: | Artikel |
Sprache: | eng |
Online-Zugang: | Volltext |
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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. |
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ISSN: | 0252-9211 |
DOI: | 10.1017/S025292110001160X |