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Monte Carlo Simulations on Possible Collimation Effects of Outflows to Fan Beam Emission of Ultraluminous Accreting X-Ray Pulsars
X. Hou, Y. You, L. Ji, R. Soria, S. N. Zhang, M. Y. Ge, L. Tao, S. Zhang, H. Feng, M. Zhou, Y. L. Tuo, L. M. Song and J. C. Wang The Astrophysical Journal 941(2) 126 (2022) https://doi.org/10.3847/1538-4357/aca2a3
A semi-analytical treatment to wind accretion in neutron star supergiant high-mass X-ray binaries – I. Eccentric orbits
XMM–Newtondiscovery of mHz quasi-periodic oscillations in the high-mass X-ray binary IGR J19140+0951
L. Sidoli, P. Esposito, S. E. Motta, G. L. Israel and G. A. Rodríguez Castillo Monthly Notices of the Royal Astronomical Society 460(4) 3637 (2016) https://doi.org/10.1093/mnras/stw1246
The Strongest Magnetic Fields in the Universe
Mikhail Revnivtsev and Sandro Mereghetti Space Sciences Series of ISSI, The Strongest Magnetic Fields in the Universe 54 299 (2016) https://doi.org/10.1007/978-1-4939-3550-5_9
Propeller effect in two brightest transient X-ray pulsars: 4U 0115+63 and V 0332+53
Roland Walter, Alexander A. Lutovinov, Enrico Bozzo and Sergey S. Tsygankov The Astronomy and Astrophysics Review 23(1) (2015) https://doi.org/10.1007/s00159-015-0082-6
Probing large-scale wind structures in Vela X–1 using off-states with INTEGRAL