Radio Study of X-ray Clusters I: A3528 --- a pre-merging cluster in the core of the Shapley Supercluster

Details Radio Study of X-ray Clusters I: A3528 --- a pre-merging cluster in the core of the Shapley Supercluster Radio Study of X-ray Clusters I: A3528 --- a pre-merging cluster in the core of the Shapley Supercluster

1997-11-27

arxiv.org/abs/astro-ph/9711330v1

Astronomy and Astrophysics

Astrophysics

LaTeX, 15 pages with 16 figures, uses mn.sty, accepted MNRAS

Scientific paper

10.1046/j.1365-8711.1998.01331.x

As part of an extensive radio--IR--optical--X-ray study of ROSAT clusters of galaxies in the Hydra region we have observed the bimodal Abell cluster A3528, located in the core of the Shapley Supercluster (z ~ 0.053), with the Molonglo Observatory Synthesis Telescope at 843 MHz and the Australia Telescope Compact Array at 1.4 and 2.4 GHz. This is part I in a series of papers which look at the relationship between the radio and X-ray emission in samples of ROSAT selected clusters. The radio source characteristics --- tailed morphologies and steep spectra --- are consistent with the effects of a dense intra-cluster medium and the pre-merging environment of A3528. In particular, we present evidence that the minor member of the radio loud dumbbell galaxy located at the centre of the northern component of A3528 is on a plunging orbit. We speculate that this orbit may have been induced by the tidal interactions between the merging components of A3528. In addition, the radio source associated with the dominant member of the dumbbell galaxy exhibits many of the characteristics of Compact Steep Spectrum sources. We argue that the radio emission from this source was triggered 10^6 yr ago by tidal interactions between the two members of the dumbbell galaxy, strengthening the argument that CSS sources are young. Re-analysis of the archive pointed PSPC data using multi-resolution filtering suggests the presence of an AGN and/or a cooling flow in the southern component of A3528.

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