Metals in the Neutral Interstellar Medium of Dwarf Star-Forming Galaxies

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dc.creatorAloisi, A.
dc.creatorHeckman, T. M.
dc.creatorHoopes, C. G.
dc.creatorLeitherer, C.
dc.creatorSavaglio, S.
dc.creatorSembach, K. R.
dc.date2004-10-04
dc.date.accessioned2026-07-07T02:14:52Z
dc.date.available2026-07-07T02:14:52Z
dc.descriptionThe determination of the metal abundances in the neutral interstellar medium of dwarf star-forming galaxies is a key step in understanding their physical and chemical evolution. This type of investigation has been possible in the last 5 years thanks to FUSE. We will give a flavor of the issues involved by presenting the work that we are performing in this astrophysical field.
dc.description3 pages. Contributed paper at the conference "Astrophysics in the Far Ultraviolet: Five Years of Discovery with FUSE", to be published by PASP, eds. Sonneborn, Moos and Andersson
dc.identifierhttps://arxiv.org/abs/astro-ph/0410072
dc.identifierhttp://arxiv.org/abs/astro-ph/0410072
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8296
dc.subjectAstrophysics
dc.titleMetals in the Neutral Interstellar Medium of Dwarf Star-Forming Galaxies
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