Mass-to-light profiles of the galaxies in the sample based on the Newtonian models. The meaning of symbols is the same as in Fig. 18. We note that the values of the mass-to-light ratios for NGC 4365 and NGC 4486 appear close because of the values of their effective radii used in this paper (see text for details); the inner points for NGC 4365 and NGC 4486 are at 0.65R_e and 0.23R_e, respectively.