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Masses of X-ray pulsars in binary systems with OB supergiants
Authors:M K Abubekerov  É A Antokhina  A M Cherepashchuk
Institution:(1) Moscow State University, Vorob’evy gory, Moscow, 119992, Russia;(2) Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow, 119992, Russia
Abstract:We describe the results of a statistical approach to analyzing the combined radial-velocity curves of X-ray binaries with OB supergiants in a Roche model, both with and without allowance for the anisotropy of the stellar wind. We present new mass estimates for the X-ray pulsars in the close binary systems Cen X-3, LMC X-4, SMC X-1, 4U 1538-52, and Vela X-1.
Keywords:
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