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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

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

Survey of period variations of superhumps in SU UMa-type dwarf novae. IX. the ninth year (2016-2017) collected times of superhump maxima for 127 SU UMa-type dwarf novae observed mainly during the 2016

Survey of period variations of superhumps in SU UMa-type dwarf novae. VIII. The eighth year (2015-2016) collected times of superhump maxima for 128 SUUMa-type dwarf novae observed mainly during the 2015

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.

Survey of period variations of superhumps in SU UMa-type dwarf novae. X. The tenth year (2017) times of superhump maxima for 102 SU UMa-type dwarf novae observed mainly during the 2017 season

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

Analysis of cataclysmic variable GSC02197-00886 evolution of the object were formed in an optically thick accretion disk with an effective temperature of T eff ≈ 45 000 K

NY Ser: Outburst Activity and Multiperiodic Processes in its Various Stages During 2014 and 2016
of the accretion disk increases (A) and a stage with developed superhumps (B). Stage A for NY Ser has been

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

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