Instabilities in Interacting Binary Stars

0511274 - FZÚ 2020 RIV US eng C - Konferenční příspěvek (zahraniční konf.)
Andronov, I.L. - Andrych, K.D. - Antoniuk, K.A. - Baklanov, A.V. - Beringer, P. - Breus, V.V. - Burwitz, V. - Chinarova, L.L. - Chochol, D. - Cook, L. M. - Cook, M. - Dubovský, P. - Godłowski, W. - Hegedüs, T. - Hoňková, K. - Hric, L. - Jeon, Y.-B. - Juryšek, Jakub - Kim, C.-H. - Kim, Y. - Kim, Y.-H. - Kolesnikov, S.V. - Kudashkina, L.S. - Kusakin, A.V. - Marsakova, V. I. - Mason, P.A. - Mašek, Martin - Mishevskiy, N. - Nelson, R.H. - Oksanen, A. - Parimucha, Š. - Park, J.-W. - Petrík, K. - Quiñones, C. - Reinsch, K. - Robertson, J.W. - Sergey, I.M. - Szpanko, M. - Tkachenko, M.G. - Tkachuk, L.G. - Traulsen, I. - Tremko, J. - Tsehmeystrenko, V.S. - Yoon, J.-N. - Zoła, S. - Shakhovskoy, N.M.
Instabilities in Interacting Binary Stars.
Non-Stable Universe: Energetic Resources, Activity Phenomena and Evolutionary Processes. San Francisco: ASTRONOMICAL SOCIETY OF THE PACIFIC, 2017 - (Mickaelian, A.; Harutyunian, H.; Nikoghosyan, E.), s. 43-50. Astronomical Society of the Pacific Conference Series, 511. ISBN 978-1-58381-906-7. ISSN 1050-3390.
[International Symposium on Non-Stable Universe: Energetic Resources, Activity Phenomena, and Evolutionary Processes. Yerevan (AM), 19.09.2016-23.09.2016]
Institucionální podpora: RVO:68378271
Klíčová slova: white-dwarf * AM Herculis * spin period * system * polar * variability * Lyrae * Cyg * Cam
Obor OECD: Astronomy (including astrophysics,space science)

The types of instability in the interacting binary stars are briefly reviewed. The project Inter-Longitude Astronomy is a series of smaller projects on concrete stars or groups of stars. It has no special funds, and is supported from resources and grants of participating organizations, when informal working groups are created. This “ILA” project is in some kind similar and complementary to other projects like WET, CBA, UkrVO, VSOLJ, BRNO, MEDUZA, AstroStatistics, where many of us collaborate. Totally we studied 1900+ variable stars of different types, including newly discovered variables. The characteristic timescale is from seconds to decades and (extrapolating) even more. The monitoring of the first star of our sample AM Her was initiated by Prof. V.P. Tsesevich (1907-1983). Since more than 358 ADS papers were published.
Trvalý link: http://hdl.handle.net/11104/0301612