The structure of blue supergiant winds and the accretion in supergiant high-mass X-ray binaries
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/398/4/2152/3060840/mnras0398-2152.pdf
Reference58 articles.
1. The theory of radiatively driven stellar winds. II - The line acceleration
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3. On the Mechanism of Accretion by Stars
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5. Are There Magnetars in High‐Mass X‐Ray Binaries? The Case of Supergiant Fast X‐Ray Transients
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