TYPE IA SUPERNOVAE

被引：1
|
作者：
Isern, J. [1 ,2 ]
Bravo, E. [3 ,4 ]
Hirschumann, A. [3 ,4 ]
机构：
[1] CSIC IEEC, Inst Ciencias Espai, Torre C-5 Parells 2n,Campus UAB, Bellaterra 08193, Spain
[2] Inst Estudis Espacials Catalunya, Bellaterra 08193, Spain
[3] UPC, Dept Fis & Engn Nucl, Barcelona 08028, Spain
[4] Inst Estudis Espacials Catalunya, Barcelona 08028, Spain
来源：
STELLAR NUCLEOSYNTHESIS 50 YEARS AFTER B2FH | 2008年 / 32卷
关键词：
D O I：
10.1051/eas:0832008
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Type Ia supernovae are thought to be the outcome of the thermonuclear explosion of a carbon-oxygen white dwarf in a close binary system. In this review we discuss the observational background, the possible progenitors, the mechanisms leading to the instability and the development of the explosion itself as well as the remaining uncertainties.
引用
收藏
页码：283 / +
页数：6
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