Diffuse bubble-like radio-halo emission in MRC 0116+111: Imprint of AGN feedback in a distant cluster of galaxies

TL;DR

This paper reports the discovery of a mini radio halo with bubble-like structure in a distant galaxy cluster, providing insights into AGN feedback and plasma bubble dynamics in cluster environments.

Contribution

It presents the first detailed observation of a bubble-like radio halo in a distant cluster, highlighting AGN feedback effects on the intracluster medium.

Findings

Discovery of a 240 kpc mini radio halo with bubble-like morphology

Similarity to M87's large-scale radio structure

Potential insights into AGN feedback mechanisms

Abstract

We report the discovery of a luminous, mini radio halo of ~240 kpc dimension at the center of a distant cluster of galaxies at redshift z = 0.131. Our optical and multi-wavelength GMRT and VLA observations reveal a highly unusual structure showing a twin bubble-like diffuse radio halo surrounding a cluster of bright elliptical galaxies; very similar to the large-scale radio structure of M87, the dominant galaxy in Virgo cluster. It presents an excellent opportunity to understand the energetics and the dynamical evolution of such radio jet inflated plasma bubbles in the hot cluster atmosphere.