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Light equation in eclipsing binary CV Boo: third body candidate in elliptical orbit

А. И. БогомазовP.K. Sternberg Astronomical Institute, M.V. Lomonosov Moscow State University, 13, Universitetskij prospect, Moscow, 119991, RussiaV. S. KozyrevaP.K. Sternberg Astronomical Institute, M.V. Lomonosov Moscow State University, 13, Universitetskij prospect, Moscow, 119991, RussiaB. L. SatovskiiV. KrushevskaNational Academy of Sciences of Ukraine, Main Astronomical Observatory, 27, Akademika Zabolotnoho ulitsa, Kyiv, 03680, UkraineYu. KuznyetsovaNational Academy of Sciences of Ukraine, Main Astronomical Observatory, 27, Akademika Zabolotnoho ulitsa, Kyiv, 03680, UkraineSh. A. EhgamberdievUlugh Beg Astronomical Institute, Uzbek Academy of Sciences, 33, Astronomicheskaya ulitsa, Tashkent, 100052, UzbekistanR. KarimovUlugh Beg Astronomical Institute, Uzbek Academy of Sciences, 33, Astronomicheskaya ulitsa, Tashkent, 100052, UzbekistanA. V. KhalikovaUlugh Beg Astronomical Institute, Uzbek Academy of Sciences, 33, Astronomicheskaya ulitsa, Tashkent, 100052, UzbekistanM. IbrahimovInstitute of Astronomy, Russian Academy of Sciences, 48, Pyatnitskaya ulitsa, Moscow, 119017, RussiaT. R. IrsmambetovaP.K. Sternberg Astronomical Institute, M.V. Lomonosov Moscow State University, 13, Universitetskij prospect, Moscow, 119991, RussiaА. В. ТутуковInstitute of Astronomy, Russian Academy of Sciences, 48, Pyatnitskaya ulitsa, Moscow, 119017, Russia

Astrophysics and Space Sciencejournal2016en

ABI

Annotatsiya

Annotatsiya mavjud emas.

Mavzular

Stellar, planetary, and galactic studies Astro and Planetary Science Gamma-ray bursts and supernovae

Identifikatorlar

DOI: 10.1007/s10509-016-2976-9

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