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Nature and chemical abundances of a sample of Lyman-α emitter objects at high redshift

ABSTRACT. We built a grid of photoionization models and compiled already available observational emission line intensities ($1000 \,\, \lt \,\, \lambda $(Å) &l

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Bibliographische Detailangaben
Hauptverfasser: Dors, Oli L. (VerfasserIn) , Agarwal, Bina (VerfasserIn) , Rydberg, Claes-Erik (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 26 June 2018
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 479, Heft: 2, Pages: 2294-2307
ISSN:1365-2966
DOI:10.1093/mnras/sty1658
Online-Zugang:Verlag, Volltext: https://doi.org/10.1093/mnras/sty1658
Verlag, Volltext: https://academic.oup.com/mnras/article/479/2/2294/5045259
Volltext
Verfasserangaben:O.L. Dors, B. Agarwal, G.F. Hägele, M.V. Cardaci, Claes-Erik Rydberg, R.A. Riffel, A.S. Oliveira, A.C. Krabbe

MARC

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