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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Bibliographische Detailangaben
Hauptverfasser: Hartwig, Tilman (VerfasserIn) , Latif, Muhammad A. (VerfasserIn) , Magg, Mattis (VerfasserIn) , Bromm, Volker (VerfasserIn) , Klessen, Ralf S. (VerfasserIn) , Glover, Simon (VerfasserIn) , Whalen, Daniel J. (VerfasserIn) , Pellegrini, Eric William (VerfasserIn) , Volonteri, Marta (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 2016 July 28
In: Monthly notices of the Royal Astronomical Society
Year: 2016, Jahrgang: 462, Heft: 2, Pages: 2184-2202
ISSN:1365-2966
DOI:10.1093/mnras/stw1775
Online-Zugang:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stw1775
Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/462/2/2184/2589885
Volltext
Verfasserangaben:Tilman Hartwig, Muhammad A. Latif, Mattis Magg, Volker Bromm, Ralf S. Klessen, Simon C.O. Glover, Daniel J. Whalen, Eric W. Pellegrini, Marta Volonteri

MARC

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