The boundaries of the GW Vir stars in the effective temperature - Surface gravity domain

被引：0

作者：

Quirion, P. -O. ^{[1
]}

Fontaine, G. ^{[1
]}

Brassard, P. ^{[1
]}

机构：

[1] Univ Montreal, Dept Phys, Montreal, PQ H3C 3J7, Canada

来源：

15TH EUROPEAN WORKSHOP ON WHITE DWARFS, PROCEEDINGS | 2007年 / 372卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We derive the theoretical red edge of the pulsating GW Vir stars by using full evolutionary calculations that involve mass loss and diffusion. We put the emphasis on the fact that the specific mass loss law used in the evolutionary computations determines the red edge's position. By combining this specific property with the observed location of the red edge in the effective temperature-surface gravity domain, we obtain interesting constraints on possible mass loss laws for PG 1159 stars.

引用

页码：649 / 654

页数：6

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