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arXiv · 2201.09629

The merging galaxy cluster Abell 3266 at low radio frequencies

S. W. Duchesne·M. Johnston-Hollitt·C. J. Riseley·I. Bartalucci·S. R. Keel
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Abstract

We present new low-frequency ($ν= 88$-216 MHz) observations of the complex merging galaxy cluster Abell 3266. These new observations are taken with the Murchison Widefield Array (MWA) in its Phase II 'extended', long-baseline configuration, offering the highest-resolution low-frequency view of the cluster to date. We report on the detection of four steep spectrum ($α\lesssim -1$ for $S_ν\propto ν^α$) extended radio sources within the cluster. We confirm the detection of a $\sim 570$ kpc radio relic to the south of the cluster, and a possible bridge of emission connecting the relic to the cluster core. We also detect two new ultra-steep-spectrum ($α\lesssim -1.7$) fossil plasma sources to the north and west of the cluster centre without associated compact radio emission. A previously detected radio galaxy in the cluster is also found to have a spectrally steepening tail with steep-spectrum components highlighted by the MWA. We do not detect a giant radio halo in the cluster. After simulating a range of radio haloes at 216 MHz we place upper limits on the radio luminosity corresponding to $\sim 7.2 \times 10^{24}$ W Hz$^{-1}$ at 150 MHz assuming the expected 500 kpc radius, up to a factor 5 lower than expected from scaling relations. Why a giant radio halo is undetected in Abell 3266 is unclear - the timeline of the merger and overall mass of the system as determined by optical and X-ray studies suggest the foundation for a hosting system.

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S. W. Duchesne, M. Johnston-Hollitt, C. J. Riseley, I. Bartalucci, S. R. Keel. 2022-01-24. The merging galaxy cluster Abell 3266 at low radio frequencies. https://doi.org/10.1093/mnras%2Fstac335

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