Compact stars and the evolution of binary systems

被引：0
|
作者：
van den Heuvel, E. P. J. [1 ]
机构：
[1] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1012 WX Amsterdam, Netherlands
来源：
BULLETIN OF THE ASTRONOMICAL SOCIETY OF INDIA | 2011年 / 39卷 / 01期
关键词：
stars: binaries: general; stars: evolution; stars: white dwarfs; stars: neutron; stars: pulsars: general; stars: supernovae: general; DELAY-TIME DISTRIBUTION; WHITE-DWARF MODELS; MAGNETIC-FIELD DECAY; NEUTRON-STAR; IA SUPERNOVAE; GENERAL-RELATIVITY; CORE COLLAPSE; PULSAR; MASS; ORIGIN;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Chandrasekhar limit is of key importance for the evolution of white dwarfs in binary systems and for the formation of neutron stars and black holes in binaries. Mass transfer can drive a white dwarf in a binary over the Chandrasekhar limit, which may lead to a Type Ia supernova (in case of a CO white dwarf) or an Accretion-Induced Collapse (AIC, in the case of an O-Ne-Mg white dwarf; and possibly also in some CO white dwarfs) which produces a neutron star. The direct formation of neutron stars or black holes out of degenerate stellar cores that exceed the Chandrasekhar limit, occurs in binaries with components that started out with masses >= 8 M-circle dot.
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页码：1 / 20
页数：20
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