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Cyclical accretion regime change in the slow X-ray pulsar 4U 0114+65 observed with Chandra
G. Sanjurjo-Ferrín, J. M. Torrejón, K. Postnov, M. Nowak, J. J. Rodes-Roca, L. Oskinova, J. Planelles-Villalva and N. Schulz Astronomy & Astrophysics 694 A192 (2025) https://doi.org/10.1051/0004-6361/202452789
Nustar observation of the binary system 4U 0114 + 65
Mohammed H Abdallah, Rasha M Samir, Denis A Leahy and Ashraf A Shaker Monthly Notices of the Royal Astronomical Society 522(3) 3271 (2023) https://doi.org/10.1093/mnras/stad1199
Catalog of the Galactic Population of X-Ray Pulsars in High-mass X-Ray Binary Systems
Determination of wind-fed model parameters of neutron stars in high-mass X-ray binaries
Ali Taani, Shigeyuki Karino, Liming Song, Chengmin Zhang and Sylvain Chaty Publications of the Astronomical Society of Australia 39 (2022) https://doi.org/10.1017/pasa.2022.32
Understanding the coexistence of spin-up and spin-down behaviours in long-period X-ray pulsars
Evolution of Spin, Orbital, and Superorbital Modulations of 4U 0114+650
Chin-Ping Hu, Yi Chou, C.-Y. Ng, Lupin Chun-Che Lin and David Chien-Chang Yen The Astrophysical Journal 844(1) 16 (2017) https://doi.org/10.3847/1538-4357/aa79a3
An XMM-Newton and NuSTAR Study of IGR J18214-1318: A Non-pulsating High-mass X-Ray Binary with a Neutron Star
Francesca M. Fornasini, John A. Tomsick, Matteo Bachetti, Roman A. Krivonos, Felix Fürst, Lorenzo Natalucci, Katja Pottschmidt and Jörn Wilms The Astrophysical Journal 841(1) 35 (2017) https://doi.org/10.3847/1538-4357/aa6ff4
XMM-Newtonspectroscopy of the accreting magnetar candidate 4U0114+65
Pragati Pradhan, Biswajit Paul, B. C. Paul, Enrico Bozzo and Tomaso M. Belloni Monthly Notices of the Royal Astronomical Society 454(4) 4467 (2015) https://doi.org/10.1093/mnras/stv2276
Specific features of the reflection effect in binary systems with compact source rotating about its axis
Virginia Trimble, Markus J. Aschwanden and Carl J. Hansen Publications of the Astronomical Society of the Pacific 118(845) 947 (2006) https://doi.org/10.1086/506157
Luminosity dependent study of the high mass X-ray binary pulsar 4U 0114 + 65 with ASCA