Binaries for LISA

被引：5

作者：

Verbunt, F

Nelemans, G

机构：

[1] Inst Astron, NL-3571 GD Utrecht, Netherlands

[2] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands

来源：

CLASSICAL AND QUANTUM GRAVITY | 2001年 / 18卷 / 19期

关键词：

D O I：

10.1088/0264-9381/18/19/306

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Binaries sufficiently compact to be observed with LISA consist of small stars, with both chosen from the following list: low-mass main sequence stars, white dwarfs, neutron stars, black holes or helium-burning cores of high-mass stars. The numbers of various types of binaries can be derived from observations, provided that observational selection effects are taken into account. They can also be derived from theoretical population synthesis, but the uncertainties are such that the resulting numbers must be gauged with observed samples.

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收藏

页码：4005 / 4011

页数：7

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