FUSE Observations of Variability in Hot-Star Winds
arXiv:astro-ph/0410082
Abstract
New constraints on the large-scale wind structures responsible for discrete absorption components are obtained from far-ultraviolet time-series observations of O supergiants in the Large Magellanic Cloud.
3 pages, 1 figure; To appear in proceedings of conference "Astrophysics in the Far Ultraviolet: Five Years of Discovery with FUSE", ASP Conf. Series (ed. Sonneborn, Moos, & Andersson)