Enigmatic sub-luminous accreting neutron stars in our galaxy

被引：0
|
作者：
Wijnands, Rudy [1 ]
机构：
[1] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands
来源：
POPULATION EXPLOSION: THE NATURE AND EVOLUTION OF X-RAY BINARIES IN DIVERSE ENVIRONMENTS | 2008年 / 1010卷
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
During the last few years a class of enigmatic sub-luminous accreting neutron stars has been found in our Galaxy. They have peak X-ray luminosities (2-10 keV) of a few times 1034 erg s(-1) to a few times 1035 erg s(-1), and both persistent and transient sources have been found. I present a short overview of our knowledge of these systems and what we can learn from them.
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页码：382 / 386
页数：5
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