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High-Redshift Quasars as Early Star Formation Probes

For a sample of 20 quasars (3 ≤ = ≤ 5) we used emission-line ratios to estimate nuclear gas metallicities and the Fe IIUV/MgII line ratio was employed to probe for effects of differential metal enrichment timescales between iron and α-elements. The quasars show enhanced...

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Foilsithe in:Revista Mexicana de Astronomía y Astrofísica
Main Authors: Matthias Dietrich, Fred Hamann
Formáid: Artigo
Teanga:Inglês
Foilsithe: Universidad Nacional Autónoma de México 2008
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Rochtain Ar Líne:https://www.redalyc.org/articulo.oa?id=57103224
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