White dwarf merging and the emission of gravitational waves

被引：0

作者：

Isern, J ^{[1
]}

García-Berro, E ^{[1
]}

Guerrero, J ^{[1
]}

Lorén-Aguilar, P ^{[1
]}

Lobo, JA ^{[1
]}

机构：

[1] Inst Estudis Espacials Catalunya, ES-08034 Barcelona, Spain

来源：

INTERACTING BINARIES: ACCRETION, EVOLUTION, AND OUTCOMES | 2005年 / 797卷

关键词：

white dwarf stars; merging stars; gravitational radiation;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We have computed, using an SPH code, the process of merging of two white dwarfs with different masses and chemical compositions. We have found that, although relatively high temperatures are attained during the most violent phase of the merging process, the thermonuclear flame is rapidly quenched. Special attention has been paid to the emission of gravitational radiation. We have found that the signature of the merging is relatively weak.

引用

页码：463 / 470

页数：8

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