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Novalike variable MV Lyr: the results of a photometric multilongitude campaignстатья
- Авторы: Katysheva N.A., Pavlenko E.P., Shugarov S.Yu, Cook L., Abolmasov P.
- Журнал: Kinematika i Fizika Nebesnykh Tel
- Номер: 3
- Год издания: 2000
- Первая страница: 393
- Последняя страница: 396
- Аннотация: The cataclysmic variable MV Lyr is nova-like variable, or ``anti-dwarf nova''. In 1979-1989 years this star similar to other ``anti-dwarf novae'' spent its time in a high brightness state (B≃ 12.5m) getting fainter by 2m-8m sometimes and returning to the ``on'' stage. But later its behaviour became non-typical for these stars. The length of its first deep minimum was 10 years. The~modern state is characterized by very strong outbursts and very frequent changes of the stages. The periods 0.128d and 0.136d were obtained for 1998 and 1999, respectively. We conclude about a~possible relation between the photometric period and brightness.
- Добавил в систему: Катышева Наталья Андреевна
Прикрепленные файлы
| № | Имя | Описание | Имя файла | Размер | Добавлен |
|---|---|---|---|---|---|
| 1. | Полный текст | kynem-3-393-2000.pdf | 706,5 КБ | 2 февраля 2016 [s_shugarov] |