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Analysis of the FF Aqr spectra
Shimanskaya N., Bikmaev I., Shimansky V.
. We determine the abundances of heavy elements in the star's atmosphere by modelling the synthetic
RT Crucis: A look into the X-ray emission of a peculiar symbiotic star
Ducci L., Doroshenko V., Suleimanov V., Nikołajuk M., Santangelo A., Ferrigno C.
© 2016 ESO.Symbiotic stars are a heterogeneous class of interacting binaries. Among them, RT Cru
The new pre-cataclysmic binary PG 2200+085
Shimansky V., Sakhibullin N., Bikmaev I., Ritter H., Suleimanov V., Borisov N., Galeev A.
detached close binary with an illumination effect or the ellipsoidal deformation of a secondary star
RXTE broadband X-ray spectra of intermediate polars and white dwarf mass estimates
Suleimanov V., Revnivtsev M., Ritter H.
Stars: novae, cataclysmic variables
Influence of Compton scattering on the broad-band X-ray spectra of intermediate polars
Suleimanov V., Poutanen J., Falanga M., Werner K.
Context. The majority of cataclysmic variables observed in the hard X-ray energy band
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.
beyond the 3: 1 resonance radius of the system again after the main superoutburst. These peculiar
The determination of white dwarf parameters in dwarf novae by optical spectral modeling
Dudnik A.A., Mitrofanova A.A., Shimansky V.V., Borisov N.V., Sakhibullin N.A.
Stars: variables: dwarf novae
The auroral radio emission of the magnetic B-type star ρ OphC
Leto P., Trigilio C., Buemi C.S., Leone F., Pillitteri I., Fossati L., Cavallaro F., Oskinova L.M., Ignace R., Krtička J., Umana G., Catanzaro G., Ingallinera A., Bufano F., Riggi S., Cerrigone L., Loru S., Schilliró F., Agliozzo C., Phillips N.M., Giarrusso M., Robrade J.
Society. The non-thermal radio emission of main-sequence early-type stars is a signature of stellar
Analysis of the FF Aqr spectra
Shimanskaya N., Bikmaev I., Shimansky V.
. We determine the abundances of heavy elements in the star's atmosphere by modelling the synthetic
Superhump evolution of WZ Sge-type dwarf nova ASASSN-14cv at rebrightening stage
Sklyanov A., Pavlenko E., Antonyuk O., Antonyuk K., Sosnovsky A., Galeev A., Pit’ N., Babina Y.
detected 8 rebrightenings of this star. Based on the light curve profiles of the rebrightenings, we

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