Schematic setup of our simulation sample. We implement two disk galaxies at a distance of 2R_200, cl from the center of a galaxy cluster while varying the impact angle Θ with respect to the cluster, resulting in an initial impact parameter d (Table 2). The initial velocity of the merging system with respect to the cluster is kept constant at V_200, cl. R_200, cl and V_200, cl refer to the virial radius and velocity of the cluster.