Carbon production from low- and intermediate-mass stars

被引：0
|
作者：
Mowlavi, N [1 ]
机构：
[1] Univ Geneva, Observ Geneve, CH-1290 Sauverny, Switzerland
来源：
ABUNDANCE PROFILES: DIAGNOSTIC TOOLS FOR GALAXY HISTORY | 1998年 / 147卷
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D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Our current knowledge of carbon production in low- and intermediate-mass stars as predicted by stellar models is presented, and compared to both the luminosity functions of carbon stars in the Magellanic Clouds and the location of nearby Tc-rich S stars in the Hertzsprug-Russel diagram. The disagreeing predictions of available AGE models concerning the issue of carbon star formation is also discussed.
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页码：166 / 170
页数：5
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