Variable and Non-spherical Stellar Winds in Luminous Hot Stars 124 Issue 2006 c) "This is

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Variable and Non-spherical Stellar Winds in Luminous Hot Stars 124 Issue 2006 c) "This isThere 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