The youngest X-ray binaries

被引：3
|
作者：
Li, Xiang-Dong [1 ,2 ]
机构：
[1] Nanjing Univ, Sch Astron & Space Sci, Nanjing 210023, Peoples R China
[2] Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210023, Peoples R China
来源：
RESEARCH IN ASTRONOMY AND ASTROPHYSICS | 2020年 / 20卷 / 10期
基金：
中国国家自然科学基金;
关键词：
accretion; accretion disks; stars; black holes; neutron; evolution; ISOLATED NEUTRON-STARS; MASS DONOR STAR; SUPERNOVA REMNANT; MAGNETIC-FIELD; POPULATION SYNTHESIS; COMPACT OBJECTS; COMPANION STAR; CIRCINUS X-1; PULSAR; DISCOVERY;
D O I：
10.1088/1674-4527/20/10/162
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Several X-ray binaries (XRBs) have been identified to be associated with supernova remnants (SNRs). Because of the short lifetimes of SNRs, this leaves them to be the youngest known XRBs. This small group of binaries provides valuable information on the formation of compact stars under the framework of massive binary evolution. In this paper we review the observational characteristics of these youngest XRBs and discuss their possible implications on the initial conditions of compact stars and their interaction with the companion stars.
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页数：8
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