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

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：

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.

引用

页码：166 / 170

页数：5