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
收藏
页码：165 / 170
页数：6
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