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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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Exploring the accretion-induced evolution of the spin period and magnetic field strength of Be/X-ray Pulsars

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Evolution implications of neutron star magnetic fields: inferred from pulsars and cyclotron lines of HMXBs

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Astrophysics and Space Science 364 (11) (2019)
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On the relationship between circumstellar disc size and X-ray outbursts in Be/X-ray binaries

I. M. Monageng, V. A. McBride, M. J. Coe, I. A. Steele and P. Reig
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Discovery of a 26.2 day period in the long-term X-ray light curve of SXP 1323: a very short orbital period for a long spin period pulsar

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Astronomy & Astrophysics 602 A81 (2017)
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Formation of Double Neutron Star Systems

T. M. Tauris, M. Kramer, P. C. C. Freire, N. Wex, H.-T. Janka, N. Langer, Ph. Podsiadlowski, E. Bozzo, S. Chaty, M. U. Kruckow, E. P. J. van den Heuvel, J. Antoniadis, R. P. Breton and D. J. Champion
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High-mass X-ray binaries in the Milky Way

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Discovery of X-ray pulsations in the Be/X-ray binary IGR J21343+4738

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On the orbital parameters of Be/X-ray binaries in the Small Magellanic Cloud

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RXTE-PCA observations of 1A 1118−61: timing and spectral studies during an outburst

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Monthly Notices of the Royal Astronomical Society 414 (2) 1023 (2011)
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