The X-ray pulsar 2A 1822−371 as a super-Eddington source
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/468/1/824/11091908/stx491.pdf
Reference63 articles.
1. THE STRUCTURE OF THE ACCRETION DISK IN THE ACCRETION DISK CORONA X-RAY BINARY 4U 1822–371 AT OPTICAL AND ULTRAVIOLET WAVELENGTHS
2. Torque reversals and pulse profile of the pulsar 4U 1626-67
3. Formation and evolution of binary and millisecond radio pulsars
4. Observations of Accreting Pulsars
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