FUSE Observations of Variability in Hot-Star Winds

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dc.creatorFullerton, A. W.
dc.creatorMassa, D. L.
dc.creatorPrinja, R. K.
dc.creatorHowarth, I. D.
dc.creatorWillis, A. J.
dc.creatorOwocki, S. P.
dc.date2004-10-04
dc.date.accessioned2026-07-07T02:14:53Z
dc.date.available2026-07-07T02:14:53Z
dc.descriptionNew 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.
dc.description3 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)
dc.identifierhttps://arxiv.org/abs/astro-ph/0410082
dc.identifierhttp://arxiv.org/abs/astro-ph/0410082
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8303
dc.subjectAstrophysics
dc.titleFUSE Observations of Variability in Hot-Star Winds
dc.typetext

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