University of Hertfordshire

From the same journal

From the same journal

Documents

  • L. Hindson
  • M. Johnston-Hollitt
  • N. Hurley-Walker
  • K. Buckley
  • J. Morgan
  • E. Carretti
  • K. S. Dwarakanath
  • M. Bell
  • G. Bernardi
  • N. D. R. Bhat
  • J. D. Bowman
  • F. Briggs
  • R. J. Cappallo
  • B. E. Corey
  • A. A. Deshpande
  • D. Emrich
  • A. Ewall-Wice
  • L. Feng
  • B. M. Gaensler
  • R. Goeke
  • And 34 others
  • L. J. Greenhill
  • B. J. Hazelton
  • D. Jacobs
  • D. L. Kaplan
  • J. C. Kasper
  • E. Kratzenberg
  • N. Kudryavtseva
  • E. Lenc
  • C. J. Lonsdale
  • M. J. Lynch
  • S. R. McWhirter
  • B. McKinley
  • D. A. Mitchell
  • M. F. Morales
  • E. Morgan
  • D. Oberoi
  • S. M. Ord
  • B. Pindor
  • T. Prabu
  • P. Procopio
  • A. R. Offringa
  • J. Riding
  • A. E. E. Rogers
  • A. Roshi
  • N. Udaya Shankar
  • K. S. Srivani
  • R. Subrahmanyan
  • S. J. Tingay
  • M. Waterson
  • R. B. Wayth
  • R. L. Webster
  • A. R. Whitney
  • A. Williams
  • C. L. Williams
View graph of relations
Original languageEnglish
Pages (from-to)330-346
Number of pages17
JournalMonthly Notices of the Royal Astronomical Society
Volume445
Issue1
Early online date25 Sep 2014
DOIs
Publication statusPublished - 21 Nov 2014

Abstract

We present the first Murchison Widefield Array observations of the well-known cluster of galaxies Abell 3667 (A3667) between 105 and 241 MHz. A3667 is one of the best known examples of a galaxy cluster hosting a double radio relic and has been reported to contain a faint radio halo and bridge. The origins of radio halos, relics and bridges is still unclear, however galaxy cluster mergers seems to be an important factor. We clearly detect the North-West (NW) and South-East (SE) radio relics in A3667 and find an integrated flux density at 149 MHz of 28.1 +/- 1.7 and 2.4 +/- 0.1 Jy, respectively, with an average spectral index, between 120 and 1400 MHz, of -0.9 +/- 0.1 for both relics. We find evidence of a spatial variation in the spectral index across the NW relic steepening towards the centre of the cluster, which indicates an ageing electron population. These properties are consistent with higher frequency observations. We detect emission that could be associated with a radio halo and bridge. How- ever, due to the presence of poorly sampled large-scale Galactic emission and blended point sources we are unable to verify the exact nature of these features.

Notes

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. © 2014 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.

ID: 10291444