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For new CCD UBVRI - observations of WZ-type star we clarified the average superhumps period, found the value of Pdot during the main outburst, studied the color variations of the CVs on different stages and time scales, found the orbital wave modulation at the quiescence, confirmed the presence of 10 rebrightenings and found the amplitude of the main outburst.
№ | Имя | Описание | Имя файла | Размер | Добавлен |
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1. | Poster_J1815.pdf | Poster_J1815.pdf | 377,3 КБ | 29 августа 2018 [s_shugarov] |