Ultraluminous X-ray sources

被引：103

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.

引用

页数：53

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