2004/10/04 by A. W. Fullerton, Fullerton, A. W., D. L. Massa +9
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0410082
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)
arxiv created 2004/10/04 · arxiv updated 2009/12/01
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.