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

Saved in:

Bibliographic Details
Main Authors:	Dors, Oli L. (Author) , Agarwal, Bina (Author) , Rydberg, Claes-Erik (Author)
Format:	Article (Journal)
Language:	English
Published:	26 June 2018
In:	Monthly notices of the Royal Astronomical Society Year: 2018, Volume: 479, Issue: 2, Pages: 2294-2307
ISSN:	1365-2966
DOI:	10.1093/mnras/sty1658
Online Access:	Verlag, Volltext: https://doi.org/10.1093/mnras/sty1658 Verlag, Volltext: https://academic.oup.com/mnras/article/479/2/2294/5045259
Author Notes:	O.L. Dors, B. Agarwal, G.F. Hägele, M.V. Cardaci, Claes-Erik Rydberg, R.A. Riffel, A.S. Oliveira, A.C. Krabbe

Description
Summary:	ABSTRACT. We built a grid of photoionization models and compiled already available observational emission line intensities ($1000 \,\, \lt \,\, \lambda $(Å) &l
Item Description:	Gesehen am 24.05.2019
Physical Description:	Online Resource
ISSN:	1365-2966
DOI:	10.1093/mnras/sty1658