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THE INFLUENCE OF POST-TRAUMATIC CHONDROPATHY ON THE FUNCTIONAL CONDITION OF KNEE JOINTS IN THE ATHLETES OF COMPETITIVE SPORTS
Kapustina N.V., Smolenskiy A.V., Sakharova M.V., Abduvosidov H.A., Zapol'nova E.N.
Investigation of the Sn2+-HCl-H2O system by Mössbauer spectroscopy
Zapol'nyi A., Khramov A., Glebov A., Delo M.
The investigation of complex formation of tin(IV) with d-tartaric acid by Mössbauer spectroscopy and polarimetry
Bashkirov S., Zapol'nyi A., Khramov A., Glebov A., Delo M., Gasisova D.
Lithium-Ion conducting oxides: Synthesis, structure, and electroconducting properties
Fortal'nova E.A., Gavrilenkov O.N., Belous A.G., Politova E.D.
OT J002656.6+284933 (CSS101212:002657+284933): An SU UMa-type dwarf nova with the longest superhump period
Kato T., Tordai T., Littlefield C., Kasai K., Shugarov S., Katysheva N., Zaostrojnykh A., Pickard R., De Miguel E., Antonyuk K., Antonyuk O., Pavlenko E., Pit N., Itoh H., Ruiz J., Isogai K., Kimura M., Wakamatsu Y., Vanmunster T., Stone G.
] superhumps among SU UMa-type dwarf novae. The object is the third known SU UMa-type dwarf nova above
Light curve modeling for time-dependent accretion disks in X-ray novae with general relativity effects taken into account
Suleimanov V., Lipunova G., Shakura N.
-disks in X-ray novae. The model is based on an analytic solution for α-disk evolution after the outburst
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.
© 2016, Pleiades Publishing, Ltd.We report the results of observations of a WZ Sge-type dwarf nova
Light curve modeling for time-dependent accretion disks in X-ray novae with general relativity effects taken into account
Suleimanov V., Lipunova G., Shakura N.
-disks in X-ray novae. The model is based on an analytic solution for α-disk evolution after the outburst
OT J002656.6+284933 (CSS101212:002657+284933): An SU UMa-type dwarf nova with the longest superhump period
Kato T., Tordai T., Littlefield C., Kasai K., Shugarov S., Katysheva N., Zaostrojnykh A., Pickard R., De Miguel E., Antonyuk K., Antonyuk O., Pavlenko E., Pit N., Itoh H., Ruiz J., Isogai K., Kimura M., Wakamatsu Y., Vanmunster T., Stone G.
] superhumps among SU UMa-type dwarf novae. The object is the third known SU UMa-type dwarf nova above
Modeling of non-stationary accretion disks in X-ray novae A 0620-00 and GRS 1124-68 during outburst
Suleimanov F., Lipunova V., Shakura I.
Aims. We address the task of modeling soft X-ray and optical light curves of X-ray novae

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