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      Studying the presence of magnetic fields in a sample of high-mass X-ray binaries

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          Abstract

          Previous circular polarization observations obtained with the ESO FOcal Reducer low dispersion spectrograpgh at the VLT in 2007-2008 revealed the presence of a weak longitudinal magnetic field on the surface of the optical component of the X-ray binary Cyg X-1, which contains a black hole and an O9.7Iab supergiant on a 5.6d orbit. In this contribution we report on recently acquired FORS2 spectropolarimetric observations of Cyg X-1 along with measurements of a few additional high-mass X-ray binaries.

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          Author and article information

          Journal
          09 December 2018
          Article
          1812.04479
          173cb2bc-9b46-4ccb-856b-6e95d2d788a4

          http://arxiv.org/licenses/nonexclusive-distrib/1.0/

          History
          Custom metadata
          5 pages, 1 table, 6 figures, to appear in IAU Symposium 346 "High-mass X-ray binaries: illuminating the passage from massive binaries to merging compact objects", 2018 August 27-31, Vienna, Austria
          astro-ph.SR astro-ph.HE

          High energy astrophysical phenomena,Solar & Stellar astrophysics
          High energy astrophysical phenomena, Solar & Stellar astrophysics

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