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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| container_title | International Astronomical Union Colloquium |
| container_volume | 111 |
| creator | Brunish, Wendee M. Willson, Lee Anne |
| description | 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. |
| doi_str_mv | 10.1017/S025292110001160X |
| format | Article |
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⊙
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12
C(α,γ)
16
O rates.</description><identifier>ISSN: 0252-9211</identifier><identifier>DOI: 10.1017/S025292110001160X</identifier><language>eng</language><ispartof>International Astronomical Union Colloquium, 1989, Vol.111, p.252-252</ispartof><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c133x-acf36591a2f9180e25904ebb8c33f550e7f87e161d5b3feba5f0388bd59cbea23</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,4009,27902,27903,27904</link.rule.ids></links><search><creatorcontrib>Brunish, Wendee M.</creatorcontrib><creatorcontrib>Willson, Lee Anne</creatorcontrib><title>Cepheid Evolution with Pulsationally-Driven Mass Loss</title><title>International Astronomical Union Colloquium</title><description>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
⊙
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12
C(α,γ)
16
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⊙
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12
C(α,γ)
16
O rates.</abstract><doi>10.1017/S025292110001160X</doi><tpages>1</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0252-9211 |
| ispartof | International Astronomical Union Colloquium, 1989, Vol.111, p.252-252 |
| issn | 0252-9211 |
| language | eng |
| recordid | cdi_crossref_primary_10_1017_S025292110001160X |
| source | Alma/SFX Local Collection |
| title | Cepheid Evolution with Pulsationally-Driven Mass Loss |
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