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- W2004343746 abstract "Abstract This paper suggests numerical model for accretion disc around neutron star of strong magnetic field in close binary system. The accretion disc is build up by constant external flux from secondary component. Conditions of magnetospheric “inclusion”, “exclussion” are imposed in aagreement which the analitical model of X-ray luminosity of such system is obtained for different velocities of disc accretion. The value of M cr i.e. the minimum admissible accretion velocity balanced by magnetic field affects significantly the evolution type." @default.
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- W2004343746 modified "2023-09-26" @default.
- W2004343746 title "Numerical model of X-ray transient" @default.
- W2004343746 doi "https://doi.org/10.1016/0273-1177(88)90448-6" @default.
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