Probing the stellar initial mass function with high-[zeta] supernovae

Abstract. The first supernovae (SNe) will soon be visible at the edge of the observable universe, revealing the birthplaces of Population III stars. With upcom

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Bibliographic Details
Main Authors:	Souza, Rafael S. de (Author) , Ishida, E. E. O. (Author) , Whalen, Daniel J. (Author) , Johnson, J. L. (Author) , Ferrara, A. (Author)
Format:	Article (Journal)
Language:	English
Published:	16 June 2014
In:	Monthly notices of the Royal Astronomical Society Year: 2014, Volume: 442, Issue: 2, Pages: 1640-1655
ISSN:	1365-2966
DOI:	10.1093/mnras/stu984
Online Access:	Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stu984 Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/442/2/1640/1747468
Author Notes:	R.S. de Souza, E.E.O. Ishida, D.J. Whalen, J.L. Johnson and A. Ferrara

Description
Summary:	Abstract. The first supernovae (SNe) will soon be visible at the edge of the observable universe, revealing the birthplaces of Population III stars. With upcom
Item Description:	Im Titel ist "Zeta" als griechischer Buchstabe dargeste Gesehen am 07.09.2020
Physical Description:	Online Resource
ISSN:	1365-2966
DOI:	10.1093/mnras/stu984