NEUTRON STARS IN THE GALACTIC CENTER

被引：8

作者：

Kim, Chunglee ^{[1
]}

Davies, Melvyn B. ^{[2
]}

机构：

[1] Ewha Womans Univ, Dept Phys, Seoul 03760, South Korea

[2] Lund Observ, Dept Astron & Theoret Phys, Box 43, SE-22100 Lund, Sweden

来源：

JOURNAL OF THE KOREAN ASTRONOMICAL SOCIETY | 2018年 / 51卷 / 05期

基金：

新加坡国家研究基金会;

关键词：

stars: neutron; pulsars: general; Galaxy: center; X-RAY BINARIES; GRAVITATIONAL-WAVES; CENTRAL PARSEC; POINT SOURCES; CATALOG; PULSARS; DISCOVERY; EVOLUTION; CLUSTER; SEARCH;

D O I：

10.5303/JKAS.2018.51.5.165

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Galactic Center is one of the most dense stellar environments in the Galaxy and is considered to be a plausible place to harbor many neutron stars. In this brief review, we summarize observational efforts in search of neutron stars within a few degrees about the Galactic Center. Up to 10% of Galactic neutron stars may reside in this central region and it is possible that more than a thousand neutron stars are located within only similar to 25 '' (<= 1 pc) about the Galactic Center. Based on observations, we discuss prospects of detecting neutron stars in the Galactic Center via gravitational waves as well as electromagnetic waves.

引用

页码：165 / 170

页数：6

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