Galaxy clusters are the largest gravitationally bound systems in the Universe, they are special laboratories where is it possible to investigate the evolution and the properties of galaxies in different environments, starting from their centre, going out to the virial radius and beyond. The properties of radio galaxies can be related to their environment and its dynamical status: nowdays, understand whether the observed properties of radio galaxies arise at formation (nature scenario), or they are an end-product of physical processes (nurture scenario) coming into play after galaxies have become part of a `group’ or a `cluster’ is difficult and much debated. We started this work, analyzing a sample of eleven Brightes Cluster Galaxies (BCGs) from ten galaxy clusters in the redshift range 0.2