Light curve modeling for time-dependent accretion disks in X-ray novae with general relativity effects taken into account-irradiation of an
accretion disk. The method is applied to the outbursts of X-ray
Nova Monocerotis 1975 (A 0620-00) and X
Light curve modeling for time-dependent accretion disks in X-ray novae with general relativity effects taken into account-irradiation of an
accretion disk. The method is applied to the outbursts of X-ray
Nova Monocerotis 1975 (A 0620-00) and X
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 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
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 Superhump evolution of WZ Sge-type dwarf nova ASASSN-14cv at rebrightening stage© 2016, Pleiades Publishing, Ltd.We report the results of observations of a WZ Sge-type dwarf
nova