Presupernova evolution and explosive nucleosynthesis of massive stars at various metallicities from Z=0 to Z=Z⊙

被引：0
|
作者：
Limongi, M [1 ]
Chieffi, A [1 ]
机构：
[1] Osserv Astron Roma, INAF, I-00136 Rome, Italy
来源：
1604-2004: SUPERNOVAE AS COSMOLOGICAL LIGHTHOUSES | 2005年 / 342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：
We present a new and homogeneous set of explosive yields for masses 13, 15, 20, 25, 30 and 35 M-circle dot and metallicities Z = 0, 10(-6), 10(-4), 10(-3), 6 (.) 10(-3), 2 (.) 10(-2). These yields are available for any choice of the mass cut upon request.
引用
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页码：122 / 125
页数：4
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