What determines the unique spectra of super-Eddington accretors? Origin of optically thick and low-temperature coronae in super-Eddington accretion flows
Author:
Affiliation:
1. Department of Astronomy, Kyoto University, Kitashirakawa-Oiwake-cho, Sakyo-ku, Kyoto, Kyoto 606-8502, Japan
2. Hakubi Center, Kyoto University, Yoshida-Honmachi, Sakyo-ku, Kyoto, Kyoto 606-8501, Japan
Abstract
Funder
JSPS
Kyoto University
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/pasj/article-pdf/73/3/630/38616714/psab023.pdf
Reference69 articles.
1. Slim accretion disks
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3. An ultraluminous X-ray source powered by an accreting neutron star
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