The Evolution of Massive Stars with Mass Loss: the H- and the He-burning Phases

被引：0

作者：

Chieffi, Alessandro ^{[1
]}

Limongi, Marco ^{[2
]}

机构：

[1] Ist Astrofis Spaziale & Fis Cosm, Ist Nazl Astrofis, I-00133 Rome, Italy

[2] Osserv Astron Roma, Ist Nazl Astrofis, I-00040 Monte Porzio Catone, Italy

来源：

JOURNAL OF THE KOREAN PHYSICAL SOCIETY | 2010年 / 56卷 / 05期

关键词：

Stars; Stellar evolution; Nucleosynthesis; WOLF-RAYET STARS; LOSS RATES; NUCLEOSYNTHESIS;

D O I：

10.3938/jkps.56.1673

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The evolution of a massive star to its final fate is strongly modified by the efficient mass loss episodes it experiences during its lifetime. In the following, we will briefly summarize how the Hand the He- burning phases depend on the adopted mass loss rate.

引用

页码：1673 / 1676

页数：4

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