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Cited article:

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The Ups and Downs of Accreting X-Ray Pulsars: Decade-long Observations with the Fermi Gamma-Ray Burst Monitor

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Mass transfer on a nuclear timescale in models of supergiant and ultra-luminous X-ray binaries

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Accretion Flows in Astrophysics

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Astrophysics and Space Science Library, Accretion Flows in Astrophysics 454 331 (2018)
https://doi.org/10.1007/978-3-319-93009-1_7

NuSTARobservations of the supergiant X-ray pulsar IGR J18027−2016: accretion from the stellar wind and possible cyclotron absorption line

Alexander A. Lutovinov, Sergey S. Tsygankov, Konstantin A. Postnov, et al.
Monthly Notices of the Royal Astronomical Society 466 (1) 593 (2017)
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Raining on black holes and massive galaxies: the top-down multiphase condensation model

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SUPER STRONG MAGNETIC FIELDS OF NEUTRON STARS IN BE X-RAY BINARIES ESTIMATED WITH NEW TORQUE AND MAGNETOSPHERE MODELS

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Bright flares in supergiant fast X-ray transients

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SPECTRAL AND TIMING NATURE OF THE SYMBIOTIC X-RAY BINARY 4U 1954+319: THE SLOWEST ROTATING NEUTRON STAR IN AN X-RAY BINARY SYSTEM

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The Astrophysical Journal 786 (2) 127 (2014)
https://doi.org/10.1088/0004-637X/786/2/127