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Fig. 14

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Photometric scaling relations in scale-free diagrams of the characteristic surface brightness of the inner and outer discs and breaks (referred to μbrkIII) with hi/ho, for real and simulated Type III S0s. Solid line: linear fit to our simulations sample. Dashed line: linear fit to the observational data by E08 and G11. Dotted line: expected relations derived from the simple observational scaling relations hiRbrkIII, hoRbrkIII, and μbrkIIIRbrkIII (see Sect. 3.6). Consult the legend in the figure. (Color version online.)

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