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Fig. 15.

image

KS test for observed late-type galaxies (gray) and dispersion-dominated (κrot <  0.5) simulated (red, green) DGs with stellar masses between 5 × 107M and 109M. The thick lines and the displayed da- and Pa-values refer to the real stellar half-mass radius distribution of the Illustris-1 simulation. The thin lines and the db- and Pb-values refer to a distribution in which all radii in the Illustris-1 simulation are divided by two (see text). The observational data are a subset of the catalog from Dabringhausen & Fellhauer (2016) including all galaxies from the Fornax, Hydra, and Centaurus cluster catalog with stellar masses between 5 × 107M and 109M.

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