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DIE FRAGE DER INTEGRATION DER UKRAINE IN DIE EU

PSYCHONEUROLOGICAL DISORDERS IN CARDIAL ACHALASIA

MARTYNOV Y.S., MALKOVA E.V., GREBENEV A.L., POROZIN G.P., MALKOV G.F.

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.

, turns out to be moderate during the source’s “high” state (when a soft blackbody emission component

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.

, turns out to be moderate during the source’s “high” state (when a soft blackbody emission component

SUBJECTS OF PRE-TRIAL PROCEEDINGS IN THE MODERN CRIMINAL PROCESS OF THE RUSSIAN FEDERATION

The subjects of pre-trial proceedings play a key role in the reproduction of the pre-trial process

Spectroscopic study of the optical counterpart to the fast X-ray transient IGR J17544-2619 based on observations at the 1.5-m RTT-150 telescope

Bikmaev I., Nikolaeva E., Shimansky V., Galeev A., Zhuchkov R., Irtuganov E., Melnikov S., Sakhibullin N., Grebenev S., Sharipova L.

that the optical star is not a supergiant as has been thought previously.

GAMMA RAYS from TYPE Ia SUPERNOVA SN 2014J

Churazov E., Sunyaev R., Isern J., Bikmaev I., Bravo E., Chugai N., Grebenev S., Jean P., Knödlseder J., Lebrun F., Kuulkers E.

and light curves are compared with a subset of models. We confirm our previous finding that the gamma

Spectroscopic study of the optical counterpart to the fast X-ray transient IGR J17544-2619 based on observations at the 1.5-m RTT-150 telescope

Bikmaev I., Nikolaeva E., Shimansky V., Galeev A., Zhuchkov R., Irtuganov E., Melnikov S., Sakhibullin N., Grebenev S., Sharipova L.

that the optical star is not a supergiant as has been thought previously.

GAMMA RAYS from TYPE Ia SUPERNOVA SN 2014J

Churazov E., Sunyaev R., Isern J., Bikmaev I., Bravo E., Chugai N., Grebenev S., Jean P., Knödlseder J., Lebrun F., Kuulkers E.

and light curves are compared with a subset of models. We confirm our previous finding that the gamma

Full orbital solution for the binary system in the northern Galactic disc microlensing event Gaia16aye

Wyrzykowski, Mróz P., Rybicki K.A., Gromadzki M., Kołaczkowski Z., Zieliński M., Zieliński P., Britavskiy N., Gomboc A., Sokolovsky K., Hodgkin S.T., Abe L., Aldi G.F., Almannaei A., Altavilla G., Al Qasim A., Anupama G.C., Awiphan S., Bachelet E., Baklş V., Baker S., Bartlett S., Bendjoya P., Benson K., Bikmaev I.F., Birenbaum G., Blagorodnova N., Blanco-Cuaresma S., Boeva S., Bonanos A.Z., Bozza V., Bramich D.M., Bruni I., Burenin R.A., Burgaz U., Butterley T., Caines H.E., Caton D.B., Calchi Novati S., Carrasco J.M., Cassan A., Epas V., Cropper M., Chruślińska M., Clementini G., Clerici A., Conti D., Conti M., Cross S., Cusano F., Damljanovic G., Dapergolas A., D'Ago G., De Bruijne J.H.J., Dennefeld M., Dhillon V.S., Dominik M., Dziedzic J., Erece O., Eselevich M.V., Esenoglu H., Eyer L., Figuera Jaimes R., Fossey S.J., Galeev A.I., Grebenev S.A., Gupta A.C., Gutaev A.G., Hallakoun N., Hamanowicz A., Han C., Handzlik B., Haislip J.B., Hanlon L., Hardy L.K., Harrison D.L., Van Heerden H.J., Hoette V.L., Horne K., Hudec R., Hundertmark M., Ihanec N., Irtuganov E.N., Itoh R., Iwanek P., Jovanovic M.D., Janulis R., Jelínek M., Jensen E., Kaczmarek Z., Katz D., Khamitov I.M., Kilic Y., Klencki J., Kolb U., Kopacki G., Kouprianov V.V., Kruszyńska K., Kurowski S., Latev G.

© ESO 2020. Gaia16aye was a binary microlensing event discovered in the direction towards

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