Exploring the nature of the Lyman-α emitter CR7

Abstract. CR7 is the brightest Lyman-α emitter observed at z > 6, which shows very strong Lyman-α and He ii 1640 Å line luminosities, but no metal-line emis

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Bibliographic Details
Main Authors: Hartwig, Tilman (Author) , Latif, Muhammad A. (Author) , Magg, Mattis (Author) , Bromm, Volker (Author) , Klessen, Ralf S. (Author) , Glover, Simon (Author) , Whalen, Daniel J. (Author) , Pellegrini, Eric William (Author) , Volonteri, Marta (Author)
Format: Article (Journal)
Language:English
Published: 2016 July 28
In: Monthly notices of the Royal Astronomical Society
Year: 2016, Volume: 462, Issue: 2, Pages: 2184-2202
ISSN:1365-2966
DOI:10.1093/mnras/stw1775
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stw1775
Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/462/2/2184/2589885
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Author Notes:Tilman Hartwig, Muhammad A. Latif, Mattis Magg, Volker Bromm, Ralf S. Klessen, Simon C.O. Glover, Daniel J. Whalen, Eric W. Pellegrini, Marta Volonteri
Description
Summary:Abstract. CR7 is the brightest Lyman-α emitter observed at z > 6, which shows very strong Lyman-α and He ii 1640 Å line luminosities, but no metal-line emis
Item Description:Im Titel ist alpha als griechischer Buchstabe dargestellt
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Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stw1775