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Radio study of X-ray clusters of galaxies—II. A1300: a post-merger cluster at z=0.31 containing a halo and a relic

Identifieur interne : 002083 ( Istex/Checkpoint ); précédent : 002082; suivant : 002084

Radio study of X-ray clusters of galaxies—II. A1300: a post-merger cluster at z=0.31 containing a halo and a relic

Auteurs : A. D. Reid [Australie] ; R. W. Hunstead [Australie] ; L. Lémonon [France] ; M. M. Pierre [France]

Source :

RBID : ISTEX:E6E3F58CF628D05897E9F07AB66DD12B08D987E6

English descriptors

Abstract

As part of an extensive radio—IR—optical—X-ray study of ROSAT clusters of galaxies in the Hydra region we have observed the Abell cluster A1300, one of the most distant (z≃ 0.31) and X-ray luminous (LX∼ 1.7 × 1045 erg s−1 cm−2, 0.1–2.4 keV) clusters in the sample, with the Molonglo Observatory Synthesis Telescope at 843 MHz and the Australia Telescope Compact Array at 1.34, 2.4, 4.8 and 8.6 GHz. Previous results in the X-ray and optical have suggested that A1300 is in a post-merging phase. We present further evidence of this with the discovery of two diffuse radio sources projected within the extended X-ray emission of A1300. These may be among the most distant radio halo and relic sources yet found. We argue that the halo source, which is seen in projection near the centre of the cluster and coincides with an extension in the X-ray surface brightness distribution, is the result of a cluster-wide process related to the merger.

Url:
DOI: 10.1046/j.1365-8711.1999.02177.x


Affiliations:


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ISTEX:E6E3F58CF628D05897E9F07AB66DD12B08D987E6

Le document en format XML

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<div type="abstract">As part of an extensive radio—IR—optical—X-ray study of ROSAT clusters of galaxies in the Hydra region we have observed the Abell cluster A1300, one of the most distant (z≃ 0.31) and X-ray luminous (LX∼ 1.7 × 1045 erg s−1 cm−2, 0.1–2.4 keV) clusters in the sample, with the Molonglo Observatory Synthesis Telescope at 843 MHz and the Australia Telescope Compact Array at 1.34, 2.4, 4.8 and 8.6 GHz. Previous results in the X-ray and optical have suggested that A1300 is in a post-merging phase. We present further evidence of this with the discovery of two diffuse radio sources projected within the extended X-ray emission of A1300. These may be among the most distant radio halo and relic sources yet found. We argue that the halo source, which is seen in projection near the centre of the cluster and coincides with an extension in the X-ray surface brightness distribution, is the result of a cluster-wide process related to the merger.</div>
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