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We present a detailed study of a close pair of clusters of galaxies, A3532and A3530, and their environments. The \textit{Chandra} X-ray image of A3532reveals presence of substructures on scales of $\sim$20$^{\prime\prime}$ in itscore. XMM-Newton maps of the clusters show excess X-ray emission from anoverlapping region between them. Spectrally determined projected temperatureand entropy maps do not show any signs of cluster scale mergers either in theoverlapping region or in any of the clusters. In A3532, however, some signs ofthe presence of galaxy scale mergers are visible e.g., anisotropic temperaturevariations in the projected thermodynamic maps, a wide angled tailed (WAT)radio source in the brighter nucleus of its dumbbell Brightest Cluster Galaxy(BCG), and a candidate X-ray cavity coincident with the northwestern extensionof the WAT source in the low-frequency radio observations. The northwesternextension in A3532 seems either a part of the WAT or an unrelated diffusesource in A3532 or in the background. There is an indication that the cool corein A3532 has been disrupted by the central AGN activity. A reanalysis of theredshift data reinforces the close proximity of the clusters. The excessemission in the overlapping region appears to be a result of tidal interactionsas the two clusters approach each other for the first time. However, we can notrule out the possibility of the excess being due to the chance superposition oftheir X-ray halos.

A cluster pair : A3532 and A3530