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The Program of Photometric Study of Cataclysmic Variables in Sternberg Astronomical Instituteстатья
- Авторы: Voloshina I., Sementsov V.
- Сборник: Proceedings of the Scientific Session "Scientific programs and Astronomy Education in SEE and Ukraine", 16-17 September 2005, Bucurest, Romania
- Серия: Romanian Astronomical Journal, Supplement
- Том: 16
- Год издания: 2006
- Место издания: Editura Academiei Romane Bucuresti Romania
- Первая страница: 165
- Последняя страница: 172
- Аннотация: Within the framework of a large observational project devoted the study of long-term photometric variability of cataclysmic variables, which has been carried out in the Sternberg Astronomical Institute, numerous photometric UBV and CCD observations were obtained. Here we present the results for most interesting objects included in our program: old novae HR Del, V603 Aql, novae V2274 Cyg and V2275 Cyg (both come to the outburst in 2001), and the very unusual recent nova V475 Sct together with two intermediate polars, V795 Her and GK Per (Nova Per 1901), the object with a very striking evolution. All observations were carried out with UBV photometer and CCD device on 60-cm telescope of the Sternberg Astronomical Institute in Crimea, beginning from 2001 up to now. The light curves of these cataclysmic variables are constructed and their color behavior is considered.
- Добавил в систему: Семенцов Валериан Никитич