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Ultraluminous X-Ray Sources-ray sources must be supercritical accretion disks like SS 433. The discovery of neutron stars in a number
Aperiodic optical variability of intermediate polars-cataclysmic variables with truncated accretion disks be well described by a model based on fluctuations propagating in a truncated accretion disk. The power
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
On the nature of pulse profile variations and timing noise in accreting millisecond pulsars profile formation accounting for the screening of the antipodal emitting spot by the accretion disk. We
Broad band variability of SS433: Accretion disk at work? can be interpreted in terms of self-similar accretion rate modulations in the accretion disk proposed
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
The boundary layer in compact binariesContext. Disk accretion onto stars leads to the formation of a boundary layer (BL) near the stellar
Change in the Orbital Period of a Binary System Due to an Outburst in a Windy Accretion Disk system and the change in its orbital period—the mass loss in the form of a wind from an accretion disk. A
Light curve modeling for time-dependent accretion disks in X-ray novae with general relativity effects taken into accountWe present a method of modeling X-ray and optical light curves of time-dependent accretion α-disks
X-ray emission from accretion disks in active galactic nucleiWe constructed a grid of relativistic models for standard high-relative-luminosity accretion α-disks
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