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Evidence for Azimuthal Asymmetry in Be Star Winds
Published online by Cambridge University Press: 12 April 2016
Abstract
Extensive IUE observations from 1987-96 have provided compelling evidence for azimuthal asymmetry in the winds of Be stars. Two identified types of wind/FUV flux behavior are briefly discussed. Interpretations based upon both nonradial pulsations and rotation of one or more active regions appear plausible.
- Type
- Section I Observations of Non-spherical Winds
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- Copyright © Springer-Verlag 1999