Massive star evolution through the ages

被引：13

作者：

Heger, A ^{[1
]}

Woosley, SE ^{[1
]}

Fryer, CL ^{[1
]}

Langer, N ^{[1
]}

机构：

[1] Univ Chicago, Enrico Fermi Inst, Dept Astron & Astrophys, Chicago, IL 60637 USA

来源：

FROM TWILIGHT TO HIGHLIGHT: THE PHYSICS OF SUPERNOVAE | 2003年

关键词：

D O I：

10.1007/10828549_1

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We review the current basic picture of the evolution of massive stars and how their evolution and structure changes as a function of initial mass. We give an overview of the fate of modern (Pop I) and primordial (Pop III) stars with emphasis on massive and very. massive stars. For single stars we show how the type of explosions, the type of remnant and their frequencies changes for different initial metallicities.

引用

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页码：3 / 12

页数：10

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