Fig. 8
Comparison between the σ0–MK plane for the S0-like remnants at z = 0 (after ~7 Gyr of passive evolution since z ~ 0.8) and observational data of local S0 galaxies. We have distinguished between the remnants resulting from prograde and retrograde encounters. The error bars in the upper left corner represent the statistical errors on both axes (see the legend below the figure).
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