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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
Ultraluminous X-Ray Sources-ray sources must be supercritical accretion disks like SS 433. The discovery of neutron stars in a number
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
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
The thickness of accretion α-disks: Theory and observationsObservations of X-ray binaries indicate substantial half-thicknesses for the accretion disks
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
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
The boundary layer in compact binariesContext. Disk accretion onto stars leads to the formation of a boundary layer (BL) near the stellar
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
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