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UV Wind Variability in B Supergiants and its Implications for Wind Structures
Published online by Cambridge University Press: 12 April 2016
Abstract
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We discuss why B supergiant winds are particularly well suited for wind studies, and present or refer to dynamic spectra which suggest the presence of disks, bifurcated winds, shock formation, rotationally modulated winds and the spontaneous generation of wind enhancements. They underscore the strength and richness of wind variability in B supergiants and the challenges these phenomena present to theoretical studies of stellar winds.
- Type
- Section III Variable Winds
- Information
- Copyright
- Copyright © Springer-Verlag 1999
References
Massa, D., Fullerton, A.W., & Prinja, R.K.
1998, in ESO Workshop on Cyclical Variability in Stellar Winds, pl21
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