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Interaction of stellar winds in the Capella binary systemстатья
Дата последнего поиска статьи во внешних источниках: 21 мая 2019 г.
- Авторы: Getman K.V., Livshits I.M.
- Журнал: Moscow University Physics Bulletin
- Том: 54
- Номер: 1
- Год издания: 1999
- Издательство: Allerton Press
- Местоположение издательства: New York, N.Y., United States
- Первая страница: 77
- Последняя страница: 81
- Аннотация: The discovery of a source of variable X-ray radiation at the nearest double star of RS CVn type (Capella) allows to evaluate the physical conditions in the source. It is apparently located in the space between the stars. The observational data are interpreted with the aid of numerical modeling of the wind interaction process. It is suggested that a dense slow wind of the active component F9 creates a gas shell around the star, after which this gas starts overflowing through the Lagrange point. The agreement between the calculated data and the observations is achieved under the condition that the loss of mass by the F9 giant exceeds 10^-9 Msun/year.
- Добавил в систему: Лившиц Илья Моисеевич