  We present new VLBI observations of Brightest Cluster Galaxies in eight
nearby Abell clusters. These data show a possible difference between Brightest
Cluster Galaxies in cool core clusters (two-sided pc scale jets) and in non
cool core clusters (one-sided pc scale jets). We suggest that this difference
could be due to the jet interaction with the surrounding medium. More data are
necessary to discuss if pc-scale properties of Brightest Cluster Galaxies are
influenced by their peculiar morphology and position in the center of rich
clusters of galaxies.
