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Light curve modeling for time-dependent accretion disks in X-ray novae with general relativity effects taken into account-irradiation of an accretion disk. The method is applied to the outbursts of X-ray Nova Monocerotis 1975 (A 0620-00) and X

Aperiodic optical variability of intermediate polars-cataclysmic variables with truncated accretion disks radii of the accretion disk in quiescent states of dwarf novae. © ESO, 2010.

Light curve modeling for time-dependent accretion disks in X-ray novae with general relativity effects taken into account-irradiation of an accretion disk. The method is applied to the outbursts of X-ray Nova Monocerotis 1975 (A 0620-00) and X

Dynamo generated magnetic configurations in accretion discs and the nature of quasi-periodic oscillations in accreting binary systems© ESO 2016.Context. Magnetic fields are important for accretion disc structure. Magnetic fields

Modeling of non-stationary accretion disks in X-ray novae A 0620-00 and GRS 1124-68 during outburst in the high/soft state.Methods. The analytic model of viscous evolution of an externally truncated accretion α-disk

Dynamo generated magnetic configurations in accretion discs and the nature of quasi-periodic oscillations in accreting binary systems© ESO 2016.Context. Magnetic fields are important for accretion disc structure. Magnetic fields

Aperiodic optical variability of intermediate polars-cataclysmic variables with truncated accretion disks radii of the accretion disk in quiescent states of dwarf novae. © ESO, 2010.

Efficiency of soft X-ray radiation reprocessing in supersoft X-ray sources of the flat inner accretion disk and the elevated disk rim is close to that of a stellar atmosphere. We have

Modeling of non-stationary accretion disks in X-ray novae A 0620-00 and GRS 1124-68 during outburst in the high/soft state.Methods. The analytic model of viscous evolution of an externally truncated accretion α-disk

Superhump evolution of WZ Sge-type dwarf nova ASASSN-14cv at rebrightening stage© 2016, Pleiades Publishing, Ltd.We report the results of observations of a WZ Sge-type dwarf nova

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