A detailed study of X-ray cavities in the intracluster environment of the cool core cluster Abell 3017

We present a detailed analysis of cool-core galaxy cluster Abell 3017, at redshift z=0.219, which has been identified to be merging with its companion 3016. This study made use X-ray Chandra, UV (GALEX), optical (ESO/VLT), mid-infrared (WISE), and radio uGMRT observations this cluster. Using various image processing techniques, such as unsharp masking, 2-d fits using Beta models, contour binning the surface brightness profiles, we show existence pair cavities, projected distance $\sim$20'' (70 kpc) $\sim$16'' (57 kpc), respectively from core Abell~3017. also detect an excess emission located 25'' $\sim$(88 south centre is likely due bulk motions in ICM either by gas sloshing or ram-pressure striping merger. find that lobes are responsible for observed cavities detected system. The lower values mid-IR WISE colour [W1-W2] [W2-W3] imply central BCG Abell~3017 star-forming galaxy. current star formation rate BCG, estimated ${\rm H\alpha}$ GALEX FUV luminosities, equal $\sim 5.06\pm 0.78$ Msun yr$^{-1}$ 9.20\pm 0.81$ yr$^{-1}$, respectively. detect, first time, phoenix $\sim$150 kpc away core, spectral index ($\alpha \!\leq\! -1.8$). report detection $\rm~Pa_\alpha$ ESO VLT SINFONI imaging data.