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Modeling the EUV spectra of optically thick boundary layers of dwarf novae in outburst© 2014 ESO. Context. Disk accretion onto weakly magnetized white dwarfs (WDs) in cataclysmic
Modeling the EUV spectra of optically thick boundary layers of dwarf novae in outburst© 2014 ESO. Context. Disk accretion onto weakly magnetized white dwarfs (WDs) in cataclysmic
The hypersoft state of Cygnus X-3: A key to jet quenching in X-ray binaries?Accretion, accretion disks
Radiation Reaction of Charged Particles Orbiting a Magnetized Schwarzschild Black Holeaccretion, accretion disks
Superhump evolution of WZ Sge-type dwarf nova ASASSN-14cv at rebrightening stageaccretion: accretion disks
X-ray variability of SS 433: Evidence for supercritical accretion of about three days suggests that the time for the passage of material through the disk is less than
High efficiency of soft X-ray radiation reprocessing in supersoft X-ray sources due to multiple scattering comes from the accretion disc rim and can only be explained by a severe thickening of the disc rim near
GK Persei and EX Hydrae: Intermediate polars with small magnetospheres by the accretion flow velocity at the white dwarf surface, which is normally close to the free-fall velocity
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
Modeling of non-stationary accretion disks in X-ray novae A 0620-00 and GRS 1124-68 during outburst in the high/soft state.Methods. The analytic model of viscous evolution of an externally truncated accretion α-disk
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