Final stages of stellar evolution and nucleosynthesis: What do we know and what would we like to know?

被引：0
|
作者：
Hillebrandt, W [1 ]
机构：
[1] Max Planck Inst Astrophys, D-85748 Garching, Germany
来源：
ASTROPHYSICS AND SPACE SCIENCE | 2002年 / 281卷 / 1-2期
关键词：
supernovae; nucleosynthesis;
D O I：
10.1023/A:1019540805389
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Recent developments in theoretical model-calculations for the synthesis of the chemical elements during late stages of stellar evolution are reviewed. Special emphasis is put on a discussion of various astrophysical sites, including core-collapse and thermonuclear supernovae, and the physics of turbulent reactive fluids. Results of numerical simulations are presented and discussed, together with new results concerning solar-system abundances as well as abundances observed in very metal-poor stars, in the context of searches for constraints on the still rather uncertain nuclear physics data and astrophysical models.
引用
收藏
页码：173 / 182
页数：10
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