Revealing the magnetic field in a distant galaxy cluster: Discovery of the complex radio emission from MACSJ0717.5 +3745

Astronomy and Astrophysics

Volumn 503, Issue 3, 2009, Pages 707-720

  Bonafede, A ^a,b   Feretti, L ^b   Giovannini, G ^a,b   Govoni, F ^c   Murgia, M ^b,c   Taylor, G B ^d   Ebeling, H ^e   Allen, S ^f   Gentile, G ^g,h   Pihlstrom Y ^d  

^a UNIVERSITY OF BOLOGNA   (Italy)

^b OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^c INAF OSSERVATORIO ASTRONOMICO DI CAGLIARI   (Italy)

^d NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^e UNIVERSITY OF HAWAII   (United States)

^f STANFORD UNIVERSITY   (United States)

^g UNIVERSITÉ LIBRE DE BRUXELLES   (Belgium)

^h GHENT UNIVERSITY   (Belgium)

Author keywords

Galaxies: clusters: general; Galaxies: clusters: individual: MACS J0717+3745; Magnetic fields; Polarization; Radiation mechanisms: non thermal

Indexed keywords

CHANDRA; CLUSTER COLLISIONS; COMPLEX CLUSTERS; GALAXIES: CLUSTERS: GENERAL; GALAXIES: CLUSTERS: INDIVIDUALS; GALAXY CLUSTERS; INTRA-CLUSTER MEDIUM; MULTI FREQUENCY; MULTIPLE FREQUENCY; MULTIRESOLUTION DATA; NONTHERMAL; RADIATION MECHANISMS: NON-THERMAL; RADIO EMISSION; RADIO HALO; THERMAL COMPONENT; VERY LARGE ARRAYS;

MAGNETIC FIELDS; POLARIZATION; TELESCOPES;

GALAXIES;

EID: 70849113718     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912520     Document Type: Article

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