Location of our S0-like remnants in the log (h_d)-log (r_e) plane, compared to the observational results (L04; W09; L10) and previous simulations of dry minor mergers (A01; EM06; EM12; EM13). Details on the symbols and colour-coding used can be found on the legend. The linear fits performed to the observational distributions of S0 and spiral galaxies are overplotted in the diagram with solid lines only when Pearson’s correlation coefficient is greater than 0.5, in this case only for S0s (ρ_S0 = 0.59, ρ_Sp = 0.21). (A colour version is available in the electronic edition.)