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

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 evolu...

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Autore principale: Wolf, Bernhard
Ente Autore: Union astronomique internationale. Colloque (Autore)
Altri autori: Stahl, Otmar (Direttore editoriale), Fullerton, Alexander W., 1959- (Direttore editoriale)
Natura: Livre numérique
Lingua:Anglais
Pubblicazione: Berlin [etc.] : Springer [20..].
Cham : Springer Nature
Serie:Lecture notes in physics 523
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Edition sous un autre format:• 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, B. Wolf, O. Stahl, A.W. Fullerton (eds.), Berlin, Springer, 1999, 1 volume (xx, 424 p.), Lecture notes in physics, 3-540-65702-9
• Variable and Non-spherical Stellar Winds in Luminous Hot Stars, Texte imprimé, 9783662142097
• Variable and Non-spherical Stellar Winds in Luminous Hot Stars, Texte imprimé, 9783662142103
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Riassunto: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.
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ISBN:9783540490623 (PDF)
ISSN:1616-6361
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