Distributions of our Type III S0-like remnants in the diagrams of μ_brkIII vs. R_brkIII, R_brkIII/R₂₅, and M_B, compared to real antitruncated S0 galaxies (E08; G11). The lines correspond to linear fits performed to the major merger remnants (solid line) and to the observational sample (dashed line). The fit performed to observations in the plane μ_brkIII – R_brkIII is one of the three simple scaling relations from which the relations observed in the rest of photometric planes can be derived (see Sect. 3.6), so it has been printed in red. Dotted line: expected relations assuming the simple scaling relations h_i ∝ R_brkIII, h_o ∝ R_brkIII, and μ_brkIII ∝ R_brkIII obtained for real data. Consult the legend in the figure. (Color version online.)