Maximum rotational velocity as a function of the central velocity dispersion for our S0-like remnants in comparison with local early-type galaxies by Davis et al. (2016) and the S0s from Table 1. The magenta triangles with an arrow denote the galaxies by Davis et al. with rotational velocities higher than the axis limit. The error bars in the upper left corner correspond to the median of the errors in both axes (see the legend below the figure). This figure is analogous to Fig. 9, but using the maximum rotational velocity measurements (see the caption there).