On the evolution and explosion of massive stars

被引:0
|
作者
Limongi, Marco [1 ]
Chieffi, Alessandro [2 ]
机构
[1] Osserv Astron Roma, INAF, Via Frascati 33, I-00040 Monte Porzio Catone, Roma, Italy
[2] Monash Univ, Ctr Stellar & Planetary Astrophys, Clayton, Vic 3800, Australia
关键词
stellar evolution; nucleosynthesis; supernovae;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We review our recent progresses on the presupernova evolution of massive stars in the range 11 - 120 M-circle dot of solar metallicity. Special attention will be devoted to the effect of the mass loss rate during the Wolf-Rayet stages in determining the structure and the physical properties of the star prior the supernova explosion. We also discuss the explosive yields and the initial mass-remnant mass relation in the framework of the kinetic bomb induced explosion and hence the contribution of these stars to the global chemical enrichment of the interstellar medium.
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页码:91 / +
页数:2
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