Cyclical Variability in Stellar Winds Proceedings of the ESO Workshop Held at Garching, Germany, 14 – 17 October 1997 / edited by Lex Kaper, Alexander W. Fullerton.

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...

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Bibliographic Details
Corporate Author: SpringerLink (Online service)
Other Authors: Kaper, Lex (Editor), Fullerton, Alexander W. (Editor)
Format: eBook
Language:English
Published: Berlin, Heidelberg : Springer Berlin Heidelberg : Imprint: Springer, 1998.
Edition:1st ed. 1998.
Series:ESO Astrophysics Symposia, European Southern Observatory,
Springer eBook Collection.
Subjects:
Online Access:Click to view e-book
Holy Cross Note:Loaded electronically.
Electronic access restricted to members of the Holy Cross Community.

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245 1 0 |a Cyclical Variability in Stellar Winds  |h [electronic resource] :  |b Proceedings of the ESO Workshop Held at Garching, Germany, 14 – 17 October 1997 /  |c edited by Lex Kaper, Alexander W. Fullerton. 
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505 0 |a 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. 
520 |a 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. 
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