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Light curve modeling for time-dependent accretion disks in X-ray novae with general relativity effects taken into account

Suleimanov V., Lipunova G., Shakura N.

-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

Revnivtsev M., Burenin R., Bikmaev I., Kniazev A., Buckley D., Pretorius M., Khamitov I., Ak T., Eker Z., Melnikov S., Crawford S., Pavlinsky M.

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

Suleimanov V., Lipunova G., Shakura N.

-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

Moss D., Sokoloff D., Suleimanov V.

© 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

Suleimanov F., Lipunova V., Shakura I.

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

Moss D., Sokoloff D., Suleimanov V.

© 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

Revnivtsev M., Burenin R., Bikmaev I., Kniazev A., Buckley D., Pretorius M., Khamitov I., Ak T., Eker Z., Melnikov S., Crawford S., Pavlinsky M.

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

Suleimanov V., Meyer F., Meyer-Hofmeister E.

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

Suleimanov F., Lipunova V., Shakura I.

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

Sklyanov A., Pavlenko E., Antonyuk O., Antonyuk K., Sosnovsky A., Galeev A., Pit’ N., Babina Y.

© 2016, Pleiades Publishing, Ltd.We report the results of observations of a WZ Sge-type dwarf nova

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