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Ultraluminous X-ray sources
DOI:10.1016/j.newar.2022.101672.png)
摘要
En 中文
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.
Keyword:
Accretion
ULXs
Black holes
Neutron stars
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