Regions of Star Formation: Chemical Issues.(Discussion Session)

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dc.creatorDiaz, Angeles I.
dc.creatorEdmunds, Mike G.
dc.creatorTerlevich, Elena
dc.date2002-11-27
dc.date.accessioned2026-07-07T02:06:34Z
dc.date.available2026-07-07T02:06:34Z
dc.descriptionThree are the main questions that were posed to the audience during this discussion session: a) Can galaxy abundances be believed?, b) What progress can we expect soon and from where? and c) Can we agree, as a community, on topics in which effort should be concentrated in the next five years? In what follows, the different contributions by people in the audience are reflected as they were said trying to convey the lively spirit that enlightened the discussion.
dc.description10 pages, 2 figures. Discussion session of the meeting "Star Formation through Time". To appear in the ASP Conference Series (2003)
dc.identifierhttps://arxiv.org/abs/astro-ph/0211593
dc.identifierhttp://arxiv.org/abs/astro-ph/0211593
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5407
dc.subjectAstrophysics
dc.titleRegions of Star Formation: Chemical Issues.(Discussion Session)
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