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Superoutburst of CR Bootis: Estimation of mass ratio of a typical AMCVn star by stage A superhumps
Isogai K., Kato T., Ohshima T., Kasai K., Oksanen A., Masumoto K., Fukushima D., Maeda K., Kawabata M., Matsuda R., Kojiguchi N., Sugiura Y., Takeda N., Matsumoto K., Itoh H., Pavlenko E., Antonyuk K., Antonyuk O., Pit N., Sosnovskij A., Baklanov A., Babina J., Sklyanov A., Kiyota S., Hambsch F., Littlefield C., Maeda Y., Cook L., Masi G., Dubovsky P., Novák R., Dvorak S., Imada A., Nogami D.
. One is a dwarf nova (DN) outbursts analogy, which suggets that the outbursts are caused by thermal
Formation of Balmer lines in the spectra of X-ray Novae
Sakhibullin N., Suleimanov V., Shimanskii V., Suleimanova S.
-illuminated accretion a disk around a Schwarzschild black hole is used as an instantaneous model for the X-ray nova
Radial dependences of physical parameters in α-disk as a consequence of two vertical structure solutions
Lipunova G., Suleimanov V.
We solve the vertical structure equations for a standard α-disk and compare the results with those
Vertical structure of the outer accretion disk in persistent low-mass X-ray binaries
Mescheryakov A., Shakura N., Suleimanov V.
accretion disk in low-mass X-ray binaries by performing a self-consistent calculation of the vertical
Survey of period variations of superhumps in SU UMa-type dwarf novae. VI. The sixth year (2013-2014)
Kato T., Dubovsky P., Kudzej I., Hambsch F., Miller I., Ohshima T., Nakata C., Kawabata M., Nishino H., Masumoto K., Mizoguchi S., Yamanaka M., Matsumoto K., Sakai D., Fukushima D., Matsuura M., Bouno G., Takenaka M., Nakagawa S., Noguchi R., Iino E., Pickard R., Maeda Y., Henden A., Kasai K., Kiyota S., Akazawa H., Imamura K., De Miguel E., Maehara H., Monard B., Pavlenko E., Antonyuk K., Pit N., Antonyuk O., Baklanov A., Ruiz J., Richmond M., Oksanen A., Harlingten C., Shugarov S., Chochol D., Masi G., Nocentini F., Schmeer P., Bolt G., Nelson P., Ulowetz J., Sabo R., Goff W., Stein W., Michel R., Dvorak S., Voloshina I., Metlov V., Katysheva N., Neustroev V., Sjoberg G., Littlefield C., Dębski B., Sowicka P., Klimaszewski M., Curyło M., Morelle E., Curtis I., Iwamatsu H., Butterworth N., Andreev M., Parakhin N., Sklyanov A., Shiokawa K., Novák R., Irsmambetova T., Itoh H., Ito Y., Hirosawa K., Denisenko D., Kochanek C., Shappee B., Stanek K., Prieto J., Itagaki K., Stubbings R.
of superhump maxima for 56 SU UMa-type dwarf novae mainly observed during the 2013-2014 season
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
Ultraluminous X-ray sources as super-Eddington accretion disks
in their accretion disks supposing the supercritical accretion. However, the strongest evidences come from optical
Ultraluminous X-Ray Sources
Fabrika S.N., Atapin K.E., Vinokurov A.S., Sholukhova O.N.
-ray sources must be supercritical accretion disks like SS 433. The discovery of neutron stars in a number
Discovery of standstills in the SU UMa-type dwarf nova NY Serpentis
Kato T., Pavlenko E., Pit N., Antonyuk K., Antonyuk O., Babina J., Baklanov A., Sosnovskij A., Belan S., Maeda Y., Sugiura Y., Sumiya S., Matsumoto H., Ito D., Nikai K., Kojiguchi N., Matsumoto K., Dubovsky P., Kudzej I., Medulka T., Wakamatsu Y., Ohnishi R., Seki T., Isogai K., Simon A., Romanjuk Y., Baransky A., Sergeev A., Godunova V., Izviekova I., Kozlov V., Sklyanov A., Zhuchkov R., Gutaev A., Ponomarenko V., Vasylenko V., Miller I., Kasai K., Dvorak S., Menzies K., De Miguel E., Brincat S., Pickard R.
© The Author(s) 2019. We found that the SU UMa-type dwarf nova NY Ser in the period gap [orbital
X-ray nova MAXI J1828-249. Evolution of the broadband spectrum during its 2013–2014 outburst
Grebenev S., Prosvetov A., Burenin R., Krivonos R., Mescheryakov A.
the outer cold regions of the accretion disk, even if the X-ray heating of its surface is taken into account

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