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Clusters of varying mass ratios can merge and the process significantlydisturbs the cluster environments and alters their global properties. Activeradio galaxies are another phenomenon that can also affect clusterenvironments. Radio jets can interact with the intra-cluster medium (ICM) andlocally affect its properties. Abell~2384 (hereafter A2384) is a unique systemthat has a dense, hot X-ray filament or bridge connecting the two unequal massclusters A2384(N) and A2384(S). The analysis of its morphology suggests thatA2384 is a post-merger system where A2384(S) has already interacted with theA2384(N), and as a result hot gas has been stripped over a ~ 1 Mpc regionbetween the two bodies. We have obtained its 325 MHz GMRT data, and we detecteda peculiar FR I type radio galaxy which is a part of the A2384(S). One of itsradio lobes interacts with the hot X-ray bridge and pushes the hot gas in theopposite direction. This results in displacement in the bridge close toA2384(S). Based on Chandra and XMM-Newton X-ray observations, we notice atemperature and entropy enhancement at the radio lobe-X-ray plasma interactionsite, which further suggests that the radio lobe is changing thermal plasmaproperties. We have also studied the radio properties of the FR I radio galaxy,and found that the size and radio luminosity of the interacting north lobe ofthe FR I galaxy are lower than those of the accompanying south lobe.

A rare case of FR I interaction with a hot X-ray bridge in the A2384 galaxy cluster