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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
First detection of two superoutbursts during the rebrightening phase of a WZ Sge-Type dwarf nova: TCP J21040470+4631129
Tampo Y., Naoto K., Isogai K., Kato T., Kimura M., Wakamatsu Y., Nogami D., Vanmunster T., Tordai T., Akazawa H., Mugas F., Nishiumi T., Béjar V.J.S., Kawauchi K., Crouzet N., Watanabe N., Casasayas-Barris N., Terada Y., Fukui A., Narita N., Palle E., Tamura M., Kusakabe N., Alonso R., Itoh H., Sokolovsky K., McIntyre B., Leahy-Mcgregor J., Brincat S.M., Dubovsky P.A., Medulka T., Kudzej I., Pavlenko E.P., Antonyuk K.A., Pit N.V., Antonyuk O.I., Babina J.V., Baklanov A.V., Sklyanov A.S., Zubareva A.M., Belinski A.A., Dodin A.V., Burlak M.A., Ikonnikova N.P., Mishin E.O., Potanin S.A., Miller I., Richmond M., Pickard R.D., Galdies C., Mizutani M., Menzies K., Stone G., Ruiz J.
rebrightenings. To induce a superoutburst during the brightening phase, the accretion disk needs to have expanded
On the nature of pulse profile variations and timing noise in accreting millisecond pulsars
Poutanen J., Ibragimov A., Annala M.
profile formation accounting for the screening of the antipodal emitting spot by the accretion disk. We
Evolution of broad-band SED during outburst rise in NS X-ray Nova Aql X-1
) in NS X-ray Nova Aql X-1 during the rise phase of a bright Fast-Rise-Exponential-Decay-type outburst
Analysis of cataclysmic variable GSC02197-00886 evolution
Mitrofanova A., Borisov N., Shimansky V.
of the object were formed in an optically thick accretion disk with an effective temperature of T eff ≈ 45 000 K
Survey of period variations of superhumps in SU UMa-type dwarf novae. VII. the seventh year (2014-2015)
Kato T., Hambsch F., Dubovsky P., Kudzej I., Monard B., Miller I., Itoh H., Kiyota S., Masumoto K., Fukushima D., Kinoshita H., Maeda K., Mikami J., Matsuda R., Kojiguchi N., Kawabata M., Takenaka M., Matsumoto K., De Miguel E., Maeda Y., Ohshima T., Isogai K., Pickard R., Henden A., Kafka S., Akazawa H., Otani N., Ishibashi S., Ogi M., Tanabe K., Imamura K., Stein W., Kasai K., Vanmunster T., Starr P., Oksanen A., Pavlenko E., Antonyuk O., Antonyuk K., Sosnovskij A., Pit N., Babina J., Sklyanov A., Novák R., Dvorak S., Michel R., Masi G., Littlefield C., Ulowetz J., Shugarov S., Golysheva P., Chochol D., Krushevska V., Ruiz J., Tordai T., Morelle E., Sabo R., Maehara H., Richmond M., Katysheva N., Hirosawa K., Goff W., Dubois F., Logie L., Rau S., Voloshina I., Andreev M., Shiokawa K., Neustroev V., Sjoberg G., Zharikov S., James N., Bolt G., Crawford T., Buczynski D., Cook L., Kochanek C., Shappee B., Stanek K., Prieto J., Denisenko D., Nishimura H., Mukai M., Kaneko S., Ueda S., Stubbings R., Moriyama M., Schmeer P., Muyllaert E.
collected times of superhump maxima for 102 SU UMa-type dwarf novae, observed mainly during the 2014
Broad band variability of SS433: Accretion disk at work?
Revnivtsev M., Fabrika S., Abolmasov P., Postnov K., Bikmaev I., Burenin R., Pavlinsky M., Sunyaev R., Khamitov I., Sakhibullin N.
can be interpreted in terms of self-similar accretion rate modulations in the accretion disk proposed
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
Change in the Orbital Period of a Binary System Due to an Outburst in a Windy Accretion Disk
Avakyan A.L., Lipunova G.V., Malanchev K.L., Shakura N.I.
system and the change in its orbital period—the mass loss in the form of a wind from an accretion disk. A
X-ray emission from accretion disks in active galactic nuclei
Suleimanov V., Ghosh K., Austin R., Ramsey B.
We constructed a grid of relativistic models for standard high-relative-luminosity accretion α-disks

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