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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 (Paperback, Softcover reprint of the original 1st ed. 1999)
Loot Price: R1,515
Discovery Miles 15 150
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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 (Paperback, Softcover reprint of the original 1st ed. 1999)
Series: Lecture Notes in Physics, 523
Expected to ship within 10 - 15 working days
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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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