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The large-scale bubble structure of the interstellar medium, and the properties of the local spiral armстатья
- Автор: Bochkarev N.G.
- Журнал: Pis'ma v Astronomicheskii Zhurnal
- Том: 10
- Год издания: 1984
- Первая страница: 184
- Последняя страница: 190
- Аннотация: It is shown that the origin of emission and dust giant bubbles is connected with the combined operation of stellar winds from Wolf-Rayet, supernova and other stars. Some arguments are given on the absence of a spiral shock in the galactic local spiral arm and on the formation inside it of compact stellar associations far from the galactic plane by the Rayleigh-Taylor instability. 8 associations in the local arm in Cygnus and a number of discrete X-ray sources projecting on the sky as a horseshoe are responsible for the observed picture of the X-ray Cygnus superbubble.
- Добавил в систему: Бочкарев Николай Геннадиевич