Probing the High-Redshift Universe with Quasar Elemental Abundances

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dc.creatorHamann, Fred
dc.date1998-12-10
dc.date.accessioned2026-07-07T02:29:35Z
dc.date.available2026-07-07T02:29:35Z
dc.descriptionThe heavy elements near QSOs provide unique measures of the star formation and chemical evolution in young galactic nuclei or pre-galactic condensations. Studies of quasar abundances also naturally address a variety of questions regarding the physics of QSO environments, including the Baldwin Effect emphasized at this meeting. Here I review the status of quasar abundance work.
dc.description19 pages LaTeX with 6 embedded figures, to appear in the proceedings of "Quasars as Standard Candles for Cosmology," (May 18-22, 1998, La Serena, Chile), ASP Conf. Series, ed. G.J. Ferland
dc.identifierhttps://arxiv.org/abs/astro-ph/9812216
dc.identifierhttp://arxiv.org/abs/astro-ph/9812216
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13531
dc.subjectAstrophysics
dc.titleProbing the High-Redshift Universe with Quasar Elemental Abundances
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