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Multiwavelength observations of Swift J0243.6+6124 from 2017 to 2022
Determination of wind-fed model parameters of neutron stars in high-mass X-ray binaries
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Fast time optical variability in Be/X-ray binaries
RX J0529.8−6556: a BeXRB pulsar with an evolving optical period and out of phase X-ray outbursts
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Multiwavelength observations of PSR J2032+4127 during the 2017 periastron passage
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Supersoft X-Ray Sources Identified with Be Binaries in the Magellanic Clouds*
Valentina Cracco, Marina Orio, Stefano Ciroi, Jay Gallagher, Ralf Kotulla and Encarni Romero-Colmenero The Astrophysical Journal 862(2) 167 (2018) https://doi.org/10.3847/1538-4357/aacefb
An application of the Ghosh & Lamb model to the accretion-powered X-ray pulsar X Persei
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Warped disks during type II outbursts in Be/X-ray binaries: evidence from optical polarimetry
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Long-term optical and X-ray variability of the Be/X-ray binary H 1145-619: Discovery of an ongoing retrograde density wave
Multiwavelength monitoring and X-ray brightening of Be X-ray binary PSR J2032+4127/MT91 213 on its approach to periastron
Wynn C. G. Ho, C.-Y. Ng, Andrew G. Lyne, et al. Monthly Notices of the Royal Astronomical Society 464(1) 1211 (2017) https://doi.org/10.1093/mnras/stw2420
High-resolution H-band Spectroscopy of Be Stars with SDSS-III/APOGEE. II. Line Profile and Radial Velocity Variability
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Optical spectroscopy of the Be/X-ray binary V850 Centauri/GX 304-1 during faint X-ray periodical activity
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