Photometric Evolution of the Orbital Light Curves of the Slow Nova V723 Cas

Авторы: Shugarov Sergei Yu, Goranskij Vitalij P., Katysheva Nataly A., Kusakin Anatolij V., Metlova Nataly V., Volkov Igor M., Chochol Drahomír, Pribulla Theodor, Karitskaja Eugenia A., Retter Alon, Shemmer Ohad, Lipkin Yiftah
Сборник: Zdeněk Kopal's Binary Star Legacy
Год издания: 2005
Место издания: Springer
Первая страница: 431
Последняя страница: 431
DOI: 10.1007/1-4020-3875-5_62
Аннотация: UBVRI photoelectric and CCD photometry of the slow nova V723 Cas obtained in the years 1995-2003 is presented. The evolution of light curves in 1-year intervals, folded with the orbital period 0.69326 days, shows an increase of the amplitude of the wave-like variations from 0.07 to 1.3 mag during the years 1997-2003. The fact that the shape and amplitude of the orbital light curves does not depend on wavelength is most probably related to the geometry of eclipses combined with the distribution of circumstellar matter in the system.
Добавил в систему: Метлова Наталья Витальевна

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