Top: Velocity dispersion distribution of the clusters hosting at least one ram pressure stripped galaxy (JType ≥ 0.3). Cluster masses, computed from the velocity dispersions assuming virialization, are shown in the top axis. The vertical lines show the velocity dispersion of well-studied clusters in the local Universe (from left to right: Fornax, Virgo, and Coma). Bottom: Frequency of galaxies of different JTypes as a function of the velocity dispersion of the hosting cluster. The symbol size is proportional to the frequency.