Discovery of diffuse radio emission at the center of the most X-ray-luminous cluster RX J1347.5-1145
Myriam Gitti (1), Chiara Ferrari (2), Wilfried Domainko (3), Luigina, Feretti (4), Sabine Schindler (2) ((1) INAF - Osservatorio Astronomico di, Bologna (2) Institute of Astro-, Particle Physics, Univ. of Innsbruck (3), Max-Planck Institute for Nuclear Physics

TL;DR
This paper reports the discovery of a diffuse radio mini-halo at the center of the X-ray luminous galaxy cluster RX J1347.5-1145, suggesting electron re-acceleration due to cooling flow and merger activity.
Contribution
First detection of a radio mini-halo in the most distant galaxy cluster, combining low and high resolution VLA data to analyze its properties and origin.
Findings
Discovery of a ~500 kpc diffuse radio source at the cluster center.
Radio emission correlates with cooling flow properties.
Morphology suggests influence of merger activity.
Abstract
We report on new VLA radio observations of the distant cluster RX J1347.5-1145, which is the most luminous in X-rays. We aim at investigating the possible presence of diffuse and extended radio emission in this very peculiar system which shows both a massive cooling flow and merging signatures. New low resolution (~18 arcsec) VLA radio observations of this cluster are combined with higher resolution (~2 arcsec) data available in the VLA archive. We discover the presence of a diffuse and extended (~500 kpc) radio source centered on the cluster, unrelated to the radio emission of the central AGN. The properties of the radio source, in particular a) its occurrence at the center of a massive cooling flow cluster, b) its total size comparable to that of the cooling region, c) its agreement with the observational trend between radio luminosity and cooling flow power, indicate that RX…
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