Ultraluminous X-ray sources

被引：56
|
作者：
King, Andrew [1 ,2 ,3 ]
Lasota, Jean-Pierre [4 ,5 ]
Middleton, Matthew [6 ]
机构：
[1] Univ Leicester, Sch Phys & Astron, Astrophys Div, Leicester LE1 7RH, England
[2] Univ Amsterdam, Astron Inst Anton Pannekoek, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands
[3] Leiden Univ, Leiden Observ, Niels Bohrweg 2, NL-2333 CA Leiden, Netherlands
[4] CNRS & Sorbonne Univ, Inst Astrophys Paris, UMR 7095, 98bis Bd Arago, F-75014 Paris, France
[5] Polish Acad Sci, Nicolaus Copernicus Astron Ctr, Ul Bartycka 18, PL-00716 Warsaw, Poland
[6] Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, England
来源：
NEW ASTRONOMY REVIEWS | 2023年 / 96卷
关键词：
Accretion; ULXs; Black holes; Neutron stars; MASS BLACK-HOLE; SUPER-EDDINGTON ACCRETION; MAGNETIZED NEUTRON-STARS; QUASI-PERIODIC OSCILLATIONS; DISC INSTABILITY MODEL; NGC; 5408; X-1; FREQUENCY-RESOLVED SPECTROSCOPY; NEAR-INFRARED COUNTERPARTS; OPTICALLY THICK ENVELOPES; HUBBLE-SPACE-TELESCOPE;
D O I：
10.1016/j.newar.2022.101672
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The study of ultraluminous X-ray sources (ULXs) has changed dramatically over the last decade. In this review we first describe the most important observations of ULXs in various wavebands , across multiple scales in space , time. We discuss recent progress and current unanswered questions. We consider the range of current theories of ULX properties in the light of this observational progress. Applying these models to neutron-star ULXs offers particularly stringent tests, as this is the unique case where the mass of the accretor is effectively fixed.
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收藏
页数：53
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