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The Superoutburst of SDSS J162520+120308 in July of 2010статья
Информация о цитировании статьи получена из
Web of Science
Дата последнего поиска статьи во внешних источниках: 27 мая 2015 г.
- Авторы: Voloshina I., Olenick R., Meziere K., Metlov V., Rovny J.
- Сборник: 9th Pacific Rim Conference on Stellar Astrophysics. Proceedings of a conference held at Lijiang, China in 14-20 April 2011
- Серия: Astronomical Society of the Pacific Conference Series
- Том: 451
- Год издания: 2011
- Первая страница: 195
- Последняя страница: 199
- Аннотация: We report photometric observations a new dwarf nova during outburst occurred in July 2010. The outburst amplitude was about 6 magnitudes and it lasted 8 days. Superhumps were detected in the light curve of this nova and the mean superhump period was measured to be Psh=0d.096042(7). During the decline the superhump period changed from 0d.0927 to 0d.1150. Our observations are consisted with SDSS J162520+120308 being a new SU UMa dwarf nova in the gap on the period distribution of cataclysmic variables.
- Добавил в систему: Метлов Владимир Георгиевич