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The Dual Radio Relics of A3667

Published online by Cambridge University Press:  26 May 2016

M. Johnston-Hollitt ,
R. W. Clay ,
R. D. Ekers ,
M. H. Wieringa  and
R. W. Hunstead
M. Johnston-Hollitt
Affiliation:
Department of Physics, University of Adelaide, SA 5005, Australia
R. W. Clay
Affiliation:
Department of Physics, University of Adelaide, SA 5005, Australia
R. D. Ekers
Affiliation:
ATNF, PO Box 76, Epping NSW 1710, Australia
M. H. Wieringa
Affiliation:
ATNF, PO Box 76, Epping NSW 1710, Australia
R. W. Hunstead
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia

Abstract

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A3667 is a remarkable cluster of galaxies possessing the two largest and brightest radio relics yet seen. It provides an important opportunity to examine the environments associated with relic production.

Type
Part 3: Clusters of Galaxies
Information
Symposium - International Astronomical Union , Volume 199: The Universe at Low Radio Frequencies , 2002 , pp. 157 - 158
Copyright
Copyright © Astronomical Society of the Pacific 2002 

References

Röttgering, H. J. A., Wieringa, M. H., Hunstead, R. W., & Ekers, R. D. 1997, MNRAS, 290, 577 CrossRefGoogle Scholar
Proust, D., Mazure, A., Sodré, L., Capelato, H & Lund, G. 1988 A&AS, 72, 415 Google Scholar
Roettiger, K., Burns, K. O. & Stone, J. M. 1999 ApJ, 518, 603 Google Scholar