Zobrazeno 1 - 9
of 9
pro vyhledávání: '"N. V. Pit'"'
Autor:
I. L. Andronov, K. A. Antoniuk, A. V. Baklanov, V. V. Breus, V. Burwitz, L. L. Chinarova, D. Chochol, P. A. Dubovsky, W. Han, T. Hegedus, A. Henden, L. Hric, Chun-Hwey Kim, Yonggi Kim, S. V. Kolesnikov, I. Kudzej, A. Liakos, P. G. Niarchos, A. Oksanen, L. Patkos, K. Petrik, N. V. Pit', N. M. Shakhovskoy, N. A. Virnina, J. Yoon, S. Zola
Publikováno v:
Odessa Astronomical Publications, Vol 23, Iss 0, Pp 8-10 (2010)
We present a review of highlights of our photometric and photo-polarimetric monitoring and mathematical modeling of interacting binary stars of different types classical, asynchronous, intermedi ate polars with 25 timescales corresponding to differ e
Externí odkaz:
https://doaj.org/article/3a1c36245b5a4bd7917c651ca8b41baa
Publikováno v:
Astrophysics. 65:483-493
Autor:
N N Kiselev, V K Rosenbush, D Petrov, I V Luk'yanyk, O V Ivanova, N V Pit, K A Antoniuk, V L Afanasiev
We present results of polarimetric, photometric, and spectral observations of the near-Earth asteroid (3200) Phaethon carried out at the 6-m BTA telescope of the Special Astrophysical Observatory and the 2.6-m and 1.25-m telescopes of the Crimean Ast
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bcbf45d2381c2700c2fdb4175053e267
http://arxiv.org/abs/2206.00911
http://arxiv.org/abs/2206.00911
Autor:
E. R. Lyumanov, K. A. Antoniuk, O. I. Antoniuk, Aleksei A. Sosnovskij, E. P. Pavlenko, N. V. Pit
Publikováno v:
Astrophysics. 63:491-503
Photometric studies of the SU UMa-type dwarf nova IRXS J161659.5+620014 have been made on the 2.6-m and 1.25-m telescopes at the Crimean Astrophysical Observatory during 2017 and 2018 in the quiescent state of the system, during normal outbursts, and
Publikováno v:
Astrophysics. 60:365-373
Results are presented from a search for periodic variations in the brightness and color indices of the active star PZ Mon based on many years of photometric data from 1992 to 2015. The photometric period derived from the entire set of observations is
Autor:
K. A. Antonyuk, S. P. Belan, N. V. Pit, N. I. Bondar, Yu. V. Pakhomov, V. I. Shenavrin, S. Yu. Gorda
Publikováno v:
Astron. Lett.
Astronomy Letters
Astronomy Letters
Based on the multiband (BVRIJHKL) photometric observations of the active red giant PZ Mon performed for the first time in the winter season of 2017-2018, we have determined the main characteristics of the spotted stellar surface in a parametric three
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9f0b7a1b967dc0ba4c4f5a8367388c9c
Autor:
A. Kh. Rzaev, A. O. Grauzhanina, T. E. Burlakova, E. V. Malogolovets, V. Ya. Solovyev, Sergey Karpov, V. V. Dyachenko, T. A. Fatkhullin, Gregory Beskin, D. A. Rastegaev, D. R. Gadelshin, A. F. Valeev, N. V. Pit, G. A. Galazutdinov, A. S. Moskvitin, G. G. Valyavin, K. A. Antonyuk, Denis Shulyak
Publikováno v:
Astrophysical Bulletin. 70:318-327
We present the results of photometric observations of the weak magnetic white dwarf WD 0009+501. The observations were carried out for two years with the 1-m telescopes of the Special and Crimean Astrophysical Observatories. As a result of these obse
Based on our photometric observations in 2015-2016 and archival photometric data for the active red giant PZ Mon, we have found the main characteristics of the stellar surface: the unspotted surface temperature Teff=4730K, the spot temperature Tspot=
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d12aec337c0e81503010baa2468c4058
http://arxiv.org/abs/1711.10242
http://arxiv.org/abs/1711.10242
Autor:
I. L. Andronov, K. A. Antoniuk, A. V. Baklanov, V. V. Breus, V. Burwitz, L. L. Chinarova, D. Chochol, P. A. Dubovsky, W. Han, T. Hegedus, A. Henden, L. Hric, Chun-Hwey Kim, Yonggi Kim, S. V. Kolesnikov, I. Kudzej, A. Liakos, P. G. Niarchos, A. Oksanen, L. Patkos, K. Petrik, N. V. Pit', N. M. Shakhovskoy, N. A. Virnina, J. Yoon, S. Zola
Publikováno v:
Odessa Astronomical Publications, Vol 23, Iss 0, Pp 8-10 (2010)
We present a review of highlights of our photometric and photo-polarimetric monitoring and mathematical modeling of interacting binary stars of different types classical, asynchronous, intermedi ate polars with 25 timescales corresponding to differ e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::1396405a7bd50fb9e25f4ecba8ffebe8
https://ruj.uj.edu.pl/xmlui/handle/item/76117
https://ruj.uj.edu.pl/xmlui/handle/item/76117