Zobrazeno 1 - 10
of 66
pro vyhledávání: '"Komarova, V. N."'
Autor:
Lipunov, V. M., Gorosabel, J., Pruzhinskaya, M. V., Postigo, A. de Ugarte, Pelassa, V., Tsvetkova, A. E., Sokolov, I. V., Kann, D. A., Xu, Dong, Gorbovskoy, E. S., Krushinski, V. V., Kornilov, V. G., Balanutsa, P. V., Boronina, S. V., Budnev, N. M., Cano, Z., Castro-Tirado, A. J., Chazov, V. V., Connaughton, V., Delvaux, C., Frederiks, D. D., Fynbo, J. F. U., Gabovich, A. V., Goldstein, A., Greiner, J., Gress, O. A., Ivanov, K. I., Jakobsson, P., Klose, S., Knust, F., Komarova, V. N., Konstantinov, E., Krylov, A. V., Kuvshinov, D. A., Kuznetsov, A. S., Lipunova, G. V., Moskvitin, A. S., Pal'shin, V. D., Pandey, S. B., Poleshchuk, V. A., Schmidl, S., Sergienko, Yu. P., Sinyakov, E. V., Schulze, S., Sokolov, V. V., Sokolova, T. N., Sparre, M., Thone, C. C., Tlatov, A. G., Tyurina, N. V., Ulanov, M. V., Yazev, S. A., Yurkov, V. V.
Publikováno v:
MNRAS, 455, 712 (2016)
We report the early discovery of the optical afterglow of gamma-ray burst (GRB) 140801A in the 137 deg$^2$ 3-$\sigma$ error-box of the Fermi Gamma-ray Burst Monitor (GBM). MASTER is the only observatory that automatically react to all Fermi alerts. G
Externí odkaz:
http://arxiv.org/abs/1510.07807
Autor:
Kumar, Brajesh, Pandey, S. B., Sahu, D. K., Vinko, J., Moskvitin, A. S., Anupama, G. C., Bhatt, V. K., Ordasi, A., Nagy, A., Sokolov, V. V., Sokolova, T. N., Komarova, V. N., Kumar, Brijesh, Bose, Subhash, Roy, Rupak, Sagar, Ram
We present the low-resolution spectroscopic and UBVRI broad-band photometric investigations of the Type IIb supernova 2011fu, discovered in UGC 01626. The photometric follow-up of this event has been initiated a few days after the explosion and cover
Externí odkaz:
http://arxiv.org/abs/1301.6538
Autor:
Inserra, C., Turatto, M., Pastorello, A., Pumo, M. L., Baron, E., Benetti, S., Cappellaro, E., Taubenberger, S., Bufano, F., Elias-Rosa, N., Zampieri, L., Harutyunyan, A., Moskvitin, A. S., Nissinen, M., Stanishev, V., Tsvetkov, D. Y., Hentunen, V. P., Komarova, V. N., Pavlyuk, N. N., Sokolov, V. V., Sokolova, T. N.
We present photometry and spectroscopy of the type IIP supernova 2009bw in UGC 2890 from few days after the outburst to 241 days. The light curve of SN 2009bw during the photospheric phase is similar to that of normal SNe IIP but with brighter peak a
Externí odkaz:
http://arxiv.org/abs/1202.0659
Autor:
Moskvitin, A. S., Fatkhullin, T. A., Sokolov, V. V., Komarova, V. N., Drake, A. J., Roy, R., Tsvetkov, D. Yu.
This paper describes the aims, objectives and first results of the observational program for the study of distant core-collapse supernovae (SNe) with redshifts z < 0.3. This work is done within the framework of an international cooperation program on
Externí odkaz:
http://arxiv.org/abs/1008.0773
Autor:
Tanvir, N. R., Fox, D. B., Levan, A. J., Berger, E., Wiersema, K., Fynbo, J. P. U., Cucchiara, A., Kruehler, T., Gehrels, N., Bloom, J. S., Greiner, J., Evans, P., Rol, E., Olivares, F., Hjorth, J., Jakobsson, P., Farihi, J., Willingale, R., Starling, R. L. C., Cenko, S. B., Perley, D., Maund, J. R., Duke, J., Wijers, R. A. M. J., Adamson, A. J., Allan, A., Bremer, M. N., Burrows, D. N., Tirado, A. J. Castro, Cavanagh, B., Postigo, A. de Ugarte, Dopita, M. A., Fatkhullin, T. A., Fruchter, A. S., Foley, R. J., Gorosabel, J., Holland, S. T., Kennea, J., Kerr, T., Klose, S., Krimm, H. A., Komarova, V. N., Kulkarni, S. R., Moskvitin, A. S., Naylor, T., Penprase, B. E., Perri, M., Podsiadlowski, P., Roth, K., Rutledge, R. E., Sakamoto, T., Schady, P., Schmidt, B. P., Soderberg, A. M., Sollerman, J., Stephens, A. W., Stratta, G., Ukwatta, T. N., Watson, D., Westra, E., Wold, T., Wolf, C.
Publikováno v:
Nature461:1254-1257,2006
It is thought that the first generations of massive stars in the Universe were an important, and quite possibly dominant, source of the ultra-violet radiation that reionized the hydrogen gas in the intergalactic medium (IGM); a state in which it has
Externí odkaz:
http://arxiv.org/abs/0906.1577
G292.0+1.8 is the Cas A-like supernova remnant containing the young pulsar PSR J1124-5916, which powers a compact torus-like pulsar wind nebula with a jet visible in X-rays. We have performed deep optical observations of the pulsar field to detect th
Externí odkaz:
http://arxiv.org/abs/0810.1930
Aims: We performed deep optical observations of the field of an old, fast-moving radio pulsar PSR B1133+16 in an attempt to detect its optical counterpart and a bow shock nebula. Methods: The observations were carried out using the direct imaging mod
Externí odkaz:
http://arxiv.org/abs/0712.0826
Autor:
Kurt, V. G., Sokolov, V. V., Fatkhullin, T. A., Komarova, V. N., Lebedev, V. S., Sokolova, T. N., Castro-Tirado, A. J., Postigo, A. de Ugarte, Gorosabel, J., Guziy, S.
Publikováno v:
Nuovo Cim.C28:521-524,2005
The earliest BTA (SAO RAS 6-m telescope) spectroscopic observations of the GRB 030329 optical transient (OT) are presented, which almost coincide in time with the "first break" ($t\sim 0.5$ day after the GRB) of the OT light curve. The beginning of s
Externí odkaz:
http://arxiv.org/abs/astro-ph/0505535
Publikováno v:
Astron.Lett. 31 (2005) 243-255; Pisma Astron.Zh. 31 (2005) 269-283
We investigated the kinematics of the pulsar wind nebula (PWN) associated with PSR B1951+32 in the old supernova remnant CTB 80 using the Fabry-Perot interferometer of the 6m Special Astrophysical Observatory telescope. In addition to the previously
Externí odkaz:
http://arxiv.org/abs/astro-ph/0503526
Autor:
Cerón, J. M. Castro, Gorosabel, J., Castro-Tirado, A. J., Sokolov, V. V., Afanasiev, V. L., Fatkhullin, T. A., Dodonov, S. N., Komarova, V. N., Cherepashchuk, A. M., Postnov, K. A., Lisenfeld, U., Greiner, J., Klose, S., Hjorth, J., Fynbo, J. P. U., Pedersen, H., Rol, E., Fliri, J., Feldt, M., Feulner, G., Andersen, M. I., Jensen, B. L., Ramírez, M. D. Pérez, Vrba, F. J., Henden, A. A., Israelian, G., Tanvir, N. R.
Publikováno v:
Astron.Astrophys. 424 (2004) 833-839
We present optical and NIR (near infrared) follow up observations of the GRB 001109 from 1 to 300 days after the burst. No transient emission was found at these wavelengths within this GRB's (Gamma Ray Burst) 50" radius BeppoSAX error box. Strong lim
Externí odkaz:
http://arxiv.org/abs/astro-ph/0406414