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The boundary layer in compact binaries
Hertfelder M., Kley W., Suleimanov V., Werner K.
Context. Disk accretion onto stars leads to the formation of a boundary layer (BL) near the stellar
Influence of rotation velocity gradient on line profiles of accretion discs of CVs
Korčáková D., Nagel T., Werner K., Suleimanov V., Votruba V.
Influence of rotation velocity gradient on line profiles of accretion discs of CVs
Eclipses during the 2010 eruption of the recurrent nova U Scorpii
Schaefer B., Pagnotta A., Lacluyze A., Reichart D., Ivarsen K., Haislip J., Nysewander M., Moore J., Oksanen A., Worters H., Sefako R., Mentz J., Dvorak S., Gomez T., Harris B., Henden A., Tan T., Templeton M., Allen W., Monard B., Rea R., Roberts G., Stein W., Maehara H., Richards T., Stockdale C., Krajci T., Sjoberg G., McCormick J., Revnivtsev M., Molkov S., Suleimanov V., Darnley M., Bode M., Handler G., Lepine S., Shara M.
of eclipse from days 41-61 (likely caused by raised rims of the accretion disk occulting the bright inner
Disk precession and quasi-periodic brightness oscillations of V603 Aql in 2001-2002
Suleimanov V., Bikmaev I., Belyakov K., Sakhibullin N., Zhukov G., Aslan Z., Kiziloglu U., Khamitov I.
in the disk precession period was caused by a change in the accretion rate in the system. V603 Aql in a state
Optical Counterparts of Ultraluminous X-Ray Sources NGC 4559 X-10 and NGC 4395 ULX-1
suggest that as the original accretion rate decreases (but nevertheless remains supercritical
Non-LTE models for neutron star atmospheres and supernova-fallback disks
Werner K., Nagel T., Rauch T., Suleimanov V.
We describe our recent progress in modeling supernova-fallback disks and neutron star (NS
The accretion flow-discrete ejection connection in GRS 1915+105
Punsly B., Rodriguez J., Trushkin S.
that the process linking accretion behavior to ejection is general from the smallest scales to high luminosity
Disk precession and quasi-periodic brightness oscillations of V603 Aql in 2001-2002
Suleimanov V., Bikmaev I., Belyakov K., Sakhibullin N., Zhukov G., Aslan Z., Kiziloglu U., Khamitov I.
in the disk precession period was caused by a change in the accretion rate in the system. V603 Aql in a state
Variations in the Period of Negative Superhumps in SU UMa-Type Dwarf Novae. I. Mn Dra (2012-2017)
Sklyanov A.S., Pavlenko E.P., Antonyuk K.A., Pit N.V., Malanushenko V.P., Shchurova A.V., Zaostrozhnykh A.M.A., Shugarov S.Y., Sosnovskij A.A., Babina J.V., Antonyuk O.I., Simon A.O., Zhuchkov R.Y., Gutaev A.G.
of the accretion disk during the time of an outburst followed by a slow decrease, in agreement with the theory
X-ray variability of SS 433: Evidence for supercritical accretion
Atapin K., Fabrika S.
of about three days suggests that the time for the passage of material through the disk is less than

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