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Cited article:
N.I. Shakura, K.A. Postnov, A.Yu. Kochetkova, L. Hjalmarsdotter
EPJ Web of Conferences, 64 (2014) 02001
Published online: 2014-01-08
This article has been cited by the following article(s):
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XMM-Newton spectroscopy of the accreting magnetar candidate 4U0114+65
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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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Raining on black holes and massive galaxies: the top-down multiphase condensation model
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Monthly Notices of the Royal Astronomical Society 466 (1) 677 (2017)
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SUPER STRONG MAGNETIC FIELDS OF NEUTRON STARS IN BE X-RAY BINARIES ESTIMATED WITH NEW TORQUE AND MAGNETOSPHERE MODELS
Chang-Sheng Shi, Shuang-Nan Zhang and Xiang-Dong Li
The Astrophysical Journal 813 (2) 91 (2015)
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Wind accretion: Theory and observations
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Accretion Flows in Astrophysics
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DOI: 10.1007/978-3-319-93009-1_7
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Mass transfer on a nuclear timescale in models of supergiant and ultra-luminous X-ray binaries
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Astronomy & Astrophysics 628 A19 (2019)
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The Ups and Downs of Accreting X-Ray Pulsars: Decade-long Observations with the Fermi Gamma-Ray Burst Monitor
C. Malacaria, P. Jenke, O. J. Roberts, et al.
The Astrophysical Journal 896 (1) 90 (2020)
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