A giant radio halo in the low luminosity X-ray cluster Abell 523

TL;DR

This paper reports the discovery of a giant radio halo in the low luminosity X-ray cluster Abell 523, challenging existing correlations and suggesting new insights into cluster merging processes and radio halo formation.

Contribution

It presents the first detailed analysis of a giant radio halo in a low X-ray luminosity cluster, indicating such halos can exist outside traditional models.

Findings

Radio halo's radio power is ten times higher than expected for its X-ray luminosity.

Radio halos can be present in low X-ray luminosity clusters.

Merging processes may be more efficient in particle reacceleration than previously thought.

Abstract

Radio halos are extended and diffuse non-thermal radio sources present at the cluster center, not obviously associated with any individual galaxy. A strong correlation has been found between the cluster X-ray luminosity and the halo radio power. We observe and analyze the diffuse radio emission present in the complex merging structure Abell 523, classified as a low luminosity X-ray cluster, to discuss its properties in the context of the halo total radio power versus X-ray luminosity correlation. We reduced VLA archive observations at 1.4 GHz to derive a deep radio image of the diffuse emission, and compared radio, optical, and X-ray data. Low-resolution VLA images detect a giant radio halo associated with a complex merging region. The properties of this new halo agree with those of radio halos in general discussed in the literature, but its radio power is about a factor of ten higher than expected on the basis of the cluster X-ray luminosity. Our study of this giant radio source demonstrates that radio halos can also be present in clusters with a low X-ray luminosity. Only a few similar cases have so far been found . This result suggests that this source represent a new class of objects, that cannot be explained by classical radio halo models. We suggest that the particle reacceleration related to merging processes is very efficient and/or the X-ray luminosity is not a good indicator of the past merging activity of a cluster.