期刊
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC
卷 129, 期 976, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/1538-3873/aa6736
关键词
accretion; accretion disks - binaries; symbiotic - novae; cataclysmic variables - stars; dwarf novae - X-rays; binaries
资金
- NASA under Astrophysics Data Analysis Program [NNX13AJ13G]
- NASA [472909, NNX13AJ13G] Funding Source: Federal RePORTER
Interacting binaries in which a white dwarf accretes material from a companion-cataclysmic variables (CVs) in which the mass donor is a Roche-lobe filling star on or near the main sequence, and symbiotic stars in which the mass donor is a late type giant-are relatively commonplace. They display a wide range of behaviors in the optical, X-rays, and other wavelengths, which still often baffle observers and theorists alike. Here I review the existing body of research on X-ray emissions from these objects for the benefits of both experts and newcomers to the field. I provide introductions to the past and current X-ray observatories, the types of known X-ray emissions from these objects, and the data analysis techniques relevant to this field. I then summarize of our knowledge regarding the X-ray emissions from magnetic CVs, non-magnetic CVs and symbiotic stars, and novae in eruption. I also discuss space density and the X-ray luminosity functions of these binaries and their contribution to the integrated X-ray emission from the Galaxy. I then discuss open questions and future prospects.
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