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Cyclical Variability in Stellar Winds: Proceedings of the ESO Workshop Held at Garching, Germany, 14 – 17 October 1997 de Lex Kaper

Cyclical Variability in Stellar Winds: Proceedings of the ESO Workshop Held at Garching, Germany, 14 – 17 October 1997: ESO Astrophysics Symposia

Editat de Lex Kaper, Alexander W. Fullerton
en Limba Engleză Hardback – 20 aug 1998
It is well known that stellar winds are variable, and the fluctuations are often cyclical in nature. This property seems to be shared by the winds of cool and hot stars, even though their outflows are driven by fundamentally different physical mechanisms. Since very similar models have been proposed to explain the cyclical wind variations observed in a wide variety of stars, the time was ripe for astrophysicists from many different sub-disciplines to present the state of the art in a concise form. The proceedings will provide a useful, up-to-date overview of the observations, interpretation, and modelling of the time-dependent mass outflows from all sorts of stars.
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Specificații

ISBN-13: 9783540648024
ISBN-10: 354064802X
Pagini: 444
Ilustrații: XXII, 418 p.
Dimensiuni: 156 x 234 x 29 mm
Greutate: 0.79 kg
Ediția:1998
Editura: Springer Berlin, Heidelberg
Colecția Springer
Seria ESO Astrophysics Symposia

Locul publicării:Berlin, Heidelberg, Germany

Public țintă

Research

Cuprins

Setting the Stage: Wind Acceleration Mechanisms.- Observations of Cyclical Wind Variability.- Processes Affecting the Emergence of the Stellar Wind.- Modelling Cyclical Variability in Stellar Outflows.- The Musicos 1996 Campaign.- Future Perspective.

Textul de pe ultima copertă

It is well known that stellar winds are variable. Recent investigations show that the observed fluctuations are often cyclical in nature. This property seems to be shared by the winds of cool and hot stars, even though the physical mechanisms driving these winds are fundamentally different. The time was ripe for astrophysicists studying different types of stars, but applying very similar models, to present the state of the art in a concise form. The proceedings will provide a useful, up-to-date overview of the observations, interpretation, and modelling of the time-dependent mass outflows from a wide variety of stars, including young, pre-main-sequence objects, solar-type stars, red supergiants, and hot, massive stars.

Caracteristici

This seems to be the first rather complete overview on the Cyclical Variability in Stellar Winds