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Conference Summary: The Demise of Spherical and Stationary Winds

Published online by Cambridge University Press:  12 April 2016

Immo Appenzeller
Immo Appenzeller*
Affiliation:
Landessternwarte, Königstuhl, D-69117 Heidelberg, Germany Max-Planck-Institut für Astronomie, Königstuhl, D 69117 Heidelberg, Germany

Abstract

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The observational evidence and the theoretical work presented at this colloquium demonstrate that significant non-spherical effects and time variations are very common phenomena in the winds from hot stars. Hence, the assumptions of spherical symmetry and stationarity, while highly successful for the theory of stellar structure, appear to be inadequate for describing and understanding the winds of hot stars. This conclusion has significant consequences for the appearance and evolution of hot stars.

Type
Session VI Evolutionary Aspects
Information
International Astronomical Union Colloquium , Volume 169: Variable and Non-spherical Stellar Winds in Luminous Hot Stars , 1999 , pp. 416 - 422
Copyright
Copyright © Springer-Verlag 1999

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