The chemical evolution of galaxies causing damped Ly$α$ absorption

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dc.creatorLindner, Ulrich
dc.creatorAlvensleben, Uta Fritze-v.
dc.creatorFricke, Klaus J.
dc.date1997-10-17
dc.date.accessioned2026-07-07T02:24:38Z
dc.date.available2026-07-07T02:24:38Z
dc.descriptionWe have compiled all available data on chemical abundances in damped Lyman alpha absorption systems for comparison with results from our combined chemical and spectrophotometric galaxy evolution models. Preliminary results from chemically consistent calculations are in agreement with observations of damped Ly$α$ systems.
dc.description2 pages Latex, 1 POSTSCRIPT figure, using psfig and conf_iap.sty To appear in Proceedings of 13th IAP (Paris) Colloquium, (July 1-5, 1997) Structure and Evolution of the IGM from QSO Absorption Lines, ed. P. Petitjean, S. Charlot
dc.identifierhttps://arxiv.org/abs/astro-ph/9710193
dc.identifierhttp://arxiv.org/abs/astro-ph/9710193
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11661
dc.subjectAstrophysics
dc.titleThe chemical evolution of galaxies causing damped Ly$α$ absorption
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