Cool core galaxy clusters are considered to be dynamically relaxed clusters with regular morphology and highly X-ray luminous central region .
However , cool core clusters can also be sites for merging events that exhibit cold fronts in X-ray and mini-halos in radio .
We present recent radio/X-ray observations of the Phoenix Cluster or SPT-CL J2344-4243 at the redshift of z = 0.596 .
Using archival Chandra X-ray observations , we detect spiraling cool gas around the cluster core as well as discover two cold fronts near the core .
It is perhaps the most distant galaxy cluster to date known to host cold fronts .
Also , we present JVLA Jansky Very Large Array \url https : //science.nrao.edu/facilities/vla 1.52 GHz observations of the minihalo , previously discovered at 610 MHz with GMRT Giant Metrewave Radio Telescope \url http : //www.gmrt.ncra.tifr.res.in observations in the center of the Phoenix galaxy cluster .
The minihalo flux density at 1.52 GHz is 9.65 \pm 0.97 mJy with the spectral index between 610 MHz and 1.52 GHz being -0.98 \pm 0.16 S _ { \nu } = \nu ^ { \alpha } where S _ { \nu } .
A possible origin of these radio sources is turbulence induced by sloshing of the gas in the cluster core .