A shock front at the radio relic of Abell 2744

Abstract. Radio relics are Mpc-scale diffuse radio sources at the peripheries of galaxy clusters which are thought to trace outgoing merger shocks. We present

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Bibliographic Details
Main Authors:	Eckert, Dominique (Author) , Jauzac, M. (Author) , Vazza, F. (Author) , Owers, M. S. (Author) , Kneib, J.-P. (Author) , Tchernin, Céline (Author) , Intema, H. (Author) , Knowles, K. (Author)
Format:	Article (Journal)
Language:	English
Published:	2016 June 16
In:	Monthly notices of the Royal Astronomical Society Year: 2016, Volume: 461, Issue: 2, Pages: 1302-1307
ISSN:	1365-2966
DOI:	10.1093/mnras/stw1435
Online Access:	Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stw1435 Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/461/2/1302/2608542
Author Notes:	D. Eckert, M. Jauzac, F. Vazza, M.S. Owers, J.-P. Kneib, C. Tchernin, H. Intema and K. Knowles

Description
Summary:	Abstract. Radio relics are Mpc-scale diffuse radio sources at the peripheries of galaxy clusters which are thought to trace outgoing merger shocks. We present
Item Description:	Gesehen am 05.05.2020
Physical Description:	Online Resource
ISSN:	1365-2966
DOI:	10.1093/mnras/stw1435