Zobrazeno 1 - 10
of 350
pro vyhledávání: '"G. Valyavin"'
Autor:
Oleg Ya. Yakovlev, Azamat F. Valeev, Gennady G. Valyavin, Alexander V. Tavrov, Vitaly N. Aitov, Guram Sh. Mitiani, Oleg I. Korablev, Gazinur A. Galazutdinov, Grigory M. Beskin, Eduard V. Emelianov, Timur A. Fatkhullin, Valery V. Vlasyuk, Vyacheslav V. Sasyuk, Alexei V. Perkov, Sergei Bondar, Tatyana E. Burlakova, Sergei N. Fabrika, Iosif I. Romanyuk
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
We used the 0.5-m robotic telescope located at the Special Astrophysical Observatory of the Russian Academy of Sciences for monitoring two square degrees of the sky with the aim of detecting new exoplanets. A dimming of the visible brightness is expe
Externí odkaz:
https://doaj.org/article/53c3cee9470340ba8724037104146c01
Publikováno v:
Astrophysical Bulletin. 78:100-104
Autor:
G. Valyavin, G. Beskin, A. Valeev, G. Galazutdinov, S. Fabrika, V. Aitov, O. Yakovlev, A. Ivanova, R. Baluev, V. Vlasyuk, Inwoo Han, S. Karpov, V. Sasyuk, A. Perkov, S. Bondar, F. Musaev, E. Emelianov, T. Fatkhullin, S. Drabek, V. Shergin, Byeong-Cheol Lee, G. Mitiani, T. Burlakova, M. Yushkin, E. Sendzikas, D. Gadelshin, L. Chmyreva, A. Beskakotov, V. Dyachenko, D. Rastegaev, A. Mitrofanova, I. Yakunin, K. Antonyuk, V. Plokhotnichenko, A. Gutaev, N. Lyapsina, V. Chernenkov, A. Biryukov, E. Ivanov, A. Belinsky, E. Sokov, A. Tavrov, O. Korablev, Myeong-Gu Park, V. Stolyarov, V. Bychkov, S. Gorda, A. Popov, A. Sobolev
Publikováno v:
Astrophysical Bulletin. 77:495-508
Autor:
V. N. Aitov, G. G. Valyavin, A. F. Valeev, G. A. Galazutdinov, A. S. Moskvitin, G. Sh. Mitiani, E. V. Emelyanov, T. A. Fatkhullin, K. A. Antonyuk, A. R. Zakinyan, S. A. Kunikin
Publikováno v:
Astrophysical Bulletin. 77:308-315
Autor:
V. N. Aitov, G. G. Valyavin, A. F. Valeev, G. Sh. Mitiani, A. S. Moskvitin, E. B. Emelyanov, T. A. Fatkhullin, K. A. Antonyuk, G. A. Galazutdinov, A. R. Zakinyan, S. A. Kunikin
Publikováno v:
Astrophysical Bulletin. 77:301-307
Publikováno v:
Odessa Astronomical Publications, Vol 14, Iss 0, Pp 215-218 (2017)
The results of a systematic magnetic survey of the brightest northern MS stars are presented. A homogeneous and representative sample of 30 upper MS stars was observed. Both fast and slow rotating normal and CP stars have been investigated by the sam
Externí odkaz:
https://doaj.org/article/3e562dd8db894befa93c722b37adc973
Autor:
M. A. Pogodin, S. E. Pavlovskii, N. G. Beskrovnaya, N. A. Drake, O. V. Kozlova, I. Yu. Alekseev, M. Borges Fenandes, C. B. Pereira, G. G. Valyavin, A. S. Miroshnichenko, S Yu. Gorda, D. L. Gorshanov
Publikováno v:
Astrophysics. 65:31-52
Autor:
O. Ya. Yakovlev, A. F. Valeev, G. G. Valyavin, A. V. Tavrov, V. N. Aitov, G. Sh. Mitiani, G. M. Beskin, O. I. Korablev, G. A. Galazutdinov, V. V. Vlasyuk, E. V. Emelyanov, T. A. Fatkhullin, V. V. Sasyuk, A. V. Perkov, S. F. Bondar’, T. E. Burlakova, S. N. Fabrika, I. I. Romanyuk
Here we present eight new candidates for exoplanets detected by the transit method at the Special Astrophysical Observatory of the Russian Academy of Sciences. Photometric observations were performed with a 50-cm robotic telescope during the second h
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::81d27ff9d2a5fc5eca5a6bb7c6618301
Publikováno v:
Odessa Astronomical Publications, Vol 18, Iss 0, Pp 135-137 (2017)
We shortly present intermidiate results of a survey for weak magnetic fields among degenerate stars (white dwarfs and hot subdwarf stars). Kilogauss upper limits of longitudinal magnetic fields are presented for several brightest DA white dwarfs and
Externí odkaz:
https://doaj.org/article/2b65b955a699486fa8dc8170f1f8475e
Autor:
V. V. Tsymbal, G. G. Valyavin, Jerzy Madej, A. O. Grauzhanina, L. V. Bychkova, V. N. Aitov, G. A. Galazutdinov, T. E. Burlakova, V. D. Bychkov
Publikováno v:
Astrophysical Bulletin. 76:297-302
—Within the program for studying the variability of slow-rotating magnetic stars, we carried out magnetic monitoring of the Ap star HD 110066 (AX CVn), the expected variability period of which was estimated as 13.4 yrs. Based on our measurements of