Variable and Non-spherical Stellar Winds in Luminous Hot Stars: Proceedings of the IAU Colloquium No. 169 Held in Heidelberg, Germany, 15–19 June 1998: 523 (Lecture Notes in Physics) - Hardcover

Hardcover

ISBN 10: 3540657029 ISBN 13: 9783540657026

Publisher: Springer-Verlag Berlin and Heidelberg GmbH & Co. K, 1999

Synopsis

There is abundant evidence that essentially all luminous hot-star winds contain time-dependent and anisotropic structures. IAU Colloquium 169 was convened to review the observations of variability and asphericity, to discuss the physical processes that might cause such behavior and to look for evolutionary consequences. The topics included OBA stars, Be stars, Wolf-Rayet stars, Be stars, and luminous blue variables (LBVs). The role played by rotation in shaping the stellar wind was a recurrent theme. Photospheric pulsations and/or magnetic fields are particularly appealing mechanisms for triggering the formation of recurrent wind structures.

Edition details

• Publisher: Springer-Verlag Berlin and Heidelberg GmbH & Co. K
• Publication date: 1999
• Language: English
• ISBN 10: 3540657029
• ISBN 13: 9783540657026
• Binding: Hardcover
• Number of pages: 428
• Editor: Wolf Bernhard, Stahl Otmar, Fullerton Alex W.