Characteristic timescales for the ram-pressure stripping (blue) and for the cluster-driven morphological transformation (red) as a function of the galaxy-to-cluster mass ratio (M_★/M_cl) derived with our analysis (Equations 3 and 5). The solid lines show the median trend, with the shaded regions showing the difference between the 16th and 84th percentiles. The dashed lines show the best-fit model. As a reference, in the horizontal axis on top we report the M_★ scale for a fixed log₁₀(M_cl/ M_⊙) = 14.7.