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Colors and patterns of black hole X-ray binary GX 339-4 temperatures of the accretion disk. We show that various spectral states of regular outbursts occupy similar
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
X-ray emission from accretion disks in active galactic nucleiWe constructed a grid of relativistic models for standard high-relative-luminosity accretion α-disks
First simultanous X-ray and optical observations of rapid variability of supercritical accretor SS433. In this model, the length of the supercritical accretion disk funnel in SS433 is ∼1012 cm.
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
Non-LTE models for neutron star atmospheres and supernova-fallback disksWe describe our recent progress in modeling supernova-fallback disks and neutron star (NS
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
The accretion flow-discrete ejection connection in GRS 1915+105 that the process linking accretion behavior to ejection is general from the smallest scales to high luminosity
Observations of Her X-1 in low states during SRG/eROSITA all-sky survey of the X-ray source when the outer parts of the accretion disk blocked the neutron star from view
Influence of rotation velocity gradient on line profiles of accretion discs of CVsInfluence of rotation velocity gradient on line profiles of accretion discs of CVs
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