Period as a function of vsin(i) for the periodic variables in common with the stars spectroscopically observed by McSwain et al. (2008). The projected rotational velocity vsin(i) is taken from those authors. The markers have the same meaning as those in Fig. 20, with the colors related to the vsin(i)/v_crit ratio according to the color scale plotted on the right of the figure, v_crit being the critical rotational velocity. The four group 2 stars are the ones having P < 1 d, the other ones belonging to group 1. Horizontal lines indicate the range of possible rotational velocities v for each star, i.e. from vsin(i) to v_crit. Our star id is indicated next to each marker, followed by the star id from McSwain & Gies (2005).