Dependence on the original S0 model of the location in the λe – ϵe diagram of the 200 random projections of our models. In each panel, we plot the progenitors and remnant resulting for models with identical initial conditions and accreted satellites, but with different initial S0 galaxies (S0b or S0c). The projections for the original S0s are represented in both panels for comparison (black dots). Blue and green dots correspond to the remnants of the models using initial S0b and S0c galaxies, respectively. Top panel: projections of the models with mass ratio 6:1, α TF = 3.5, small pericentre distance, and prograde orbits. Bottom panel: projections of the models with mass ratio 6:1, α TF = 3.5, small pericentre distance, and retrograde orbits. The legend for the lines is the same as in Fig. 2. The error bars in the left upper corner of each frame represent the typical errors in both axes. (This figure is available in color in electronic form.)
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