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Radial dependences of physical parameters in α-disk as a consequence of two vertical structure solutions
Lipunova G., Suleimanov V.
We solve the vertical structure equations for a standard α-disk and compare the results with those
Vertical structure of the outer accretion disk in persistent low-mass X-ray binaries
Mescheryakov A., Shakura N., Suleimanov V.
accretion disk in low-mass X-ray binaries by performing a self-consistent calculation of the vertical
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.
be well described by a model based on fluctuations propagating in a truncated accretion disk. The power
Vertical structure of the outer accretion disk in persistent low-mass X-ray binaries
Mescheryakov A., Shakura N., Suleimanov V.
accretion disk in low-mass X-ray binaries by performing a self-consistent calculation of the vertical
Radial dependences of physical parameters in α-disk as a consequence of two vertical structure solutions
Lipunova G., Suleimanov V.
We solve the vertical structure equations for a standard α-disk and compare the results with those
Non-LTE models for neutron star atmospheres and supernova-fallback disks
Werner K., Nagel T., Rauch T., Suleimanov V.
We describe our recent progress in modeling supernova-fallback disks and neutron star (NS
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
On the nature of pulse profile variations and timing noise in accreting millisecond pulsars
Poutanen J., Ibragimov A., Annala M.
profile formation accounting for the screening of the antipodal emitting spot by the accretion disk. We
Ultraluminous X-ray sources as super-Eddington accretion disks
in their accretion disks supposing the supercritical accretion. However, the strongest evidences come from optical
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.
be well described by a model based on fluctuations propagating in a truncated accretion disk. The power

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