Supergiant fast X-ray transients versus classical supergiant high mass X-ray binaries: Does the difference lie in the companion wind?

Author: Pradhan P.   Bozzo E.   Paul B.  

Publisher: Edp Sciences

E-ISSN: 1432-0746|610|issue|A50-A50

ISSN: 0004-6361

Source: Astronomy & Astrophysics, Vol.610, Iss.issue, 2018-02, pp. : A50-A50

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