Titlebook: Instability and Variability of Hot-Star Winds; Proceedings of an In Anthony F. J. Moffat,Stanley P. Owocki,Nicole St-L Conference proceedin

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Monitoring the Winds of Hot Stars with HST/GHRSWe present observations obtained with the Goddard High Resolution Spectrograph (GHRS) of three 0-type stars: ξ per (07 III), λ Cep (06 Iaf) and 10 Lac (09 V). These observations show evidence of instabilities in the winds of all three stars, although not necessarily those expected from current models of structured winds.

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Wolf-Rayet Stars as (Potentially) Fast Rotators with Rotationally-Induced InstabilityIndirect lines of evidence for fast axial rotation of WR stars are described, such as: a) elongated cavities around WRs; b) flattening of WR winds; c) solar-like flares of WRs; d) non-radial pulsations of the WR wind in the presence of a massive companion in a binary system.

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https://doi.org/10.1007/978-94-011-0315-2astrophysics; interstellar matter; simulation; stellar; turbulence; universe

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