Heavy Elements in QSOs: Star Formation and Galaxy Evolution at High Redshifts

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dc.creatorHamann, Fred
dc.date1998-09-29
dc.date.accessioned2026-07-07T02:28:08Z
dc.date.available2026-07-07T02:28:08Z
dc.descriptionIntrinsic emission and absorption lines of QSOs provide several independent probes of the metal abundances in QSO environments. They indicate that the metallicities are typically solar or higher out to redshifts z > 4. These results support models of galaxy evolution where galactic nuclei, or dense condensations that later become galactic nuclei, form stars and evolve quickly at redshifts higher than the QSOs themselves.
dc.description4 pages LaTeX, proceedings for "The Birth of Galaxies", June 1998, Blois, France
dc.identifierhttps://arxiv.org/abs/astro-ph/9809386
dc.identifierhttp://arxiv.org/abs/astro-ph/9809386
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12989
dc.subjectAstrophysics
dc.titleHeavy Elements in QSOs: Star Formation and Galaxy Evolution at High Redshifts
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