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An analysis of the halo and relic radio emission from Abell 3376 from Murchison widefield array observations

George, L.T.; Dwarakanath, K S; Johnston-Hollitt, M; Hurley-Walker, Natasha; Hindson, L; Kapinska, A.D.; Tingay, Steven; Bell, M.; Callingham, J; For, Bi-Qing; Hancock, P.J.; Lenc, E; McKinley, B.; Morgan, John; Offringa, Andre; Procopio, P.; Staveley-Smith, Lister; Wayth, Randall; Wu, Chen; Zheng, Q.; Bernardi, G; Bowman, J D; Briggs, Franklin; Cappallo, Roger C; Corey, Brian E; Deshpande, Avinash; Emrich, David; Goeke, R; Greenhill, Lincoln; Hazelton, B; Kaplan, D L; Kasper, J.C.; Kratzenberg, Eric; Lonsdale, Colin J; Lynch, Mervyn J; McWhirter, S.R.; Mitchell, Daniel A; Morales, Miguel F; Morgan, Edward H; Oberoi, D; Ord, S M; Prabu, T; Rogers, Alan; Roshi, A.; Udaya Shankar, N.; Srivani, K. S.; Subrahmanyan, R.; Waterson, M; Webster, Rachel L; Whitney, Alan; Williams, Anne M.; Williams, Christopher L


We have carried out multiwavelength observations of the nearby (z = 0.046) rich, merging galaxy cluster Abell 3376 with the Murchison Widefield Array (MWA). As a part of the GaLactic and Extragalactic All-sky MWA Survey, this cluster was observed at 88, 118, 154, 188, and 215 MHz. The known radio relics, towards the eastern and western peripheries of the cluster, were detected at all the frequencies. The relics, with a linear extent of ~1 Mpc each, are separated by ~2 Mpc. Combining the current...[Show more]

CollectionsANU Research Publications
Date published: 2015
Type: Journal article
Source: Monthly Notices of the Royal Astronomical Society
DOI: 10.1093/mnras/stv1152


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