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Supercritical accretion disks in ultraluminous X-ray sources and SS 433 hot winds from the accretion disks with nearly normal hydrogen content, which have similar physical
NuSTAR and Swift Observations of the Ultraluminous X-Ray Source IC 342 X-1 in 2016: Witnessing Spectral Evolution-luminosity state of IC 342 X-1. The observed spectrum has a broader profile than the multi-color disk blackbody
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
Supercritical accretion disks in ultraluminous X-ray sources and SS 433 hot winds from the accretion disks with nearly normal hydrogen content, which have similar physical
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
Superhumps linked to X-ray emission: The superoutbursts of SSS J122221.7-311525 and GW Lib layer for the first time, and suggests that models for accretion discs in high mass ratio accreting
Dwarf nova EZ Lyncis second visit to instability stripAccretion disks
Evidence for the radiation-pressure dominated accretion disk in bursting pulsar GRO J1744-28 using timing analysis-II X-ray bursts, allowing studies of the interaction of the accretion disk with the magnetosphere
Burst-induced coronal cooling in GS 1826-24: The clock wagging its tail of the hot inner accretion flow that surrounds the bursting neutron star. Given that GS 1826-24 remained
OT J002656.6+284933 (CSS101212:002657+284933): An SU UMa-type dwarf nova with the longest superhump periodaccretion, accretion disks
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