Fig. 5
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Minimum pericentre distance (in units of R200 of the cluster) as a function of the number of orbits performed by each galaxy, for the sample of massive satellite galaxies. The colours (and size) indicate the stellar-to-total mass ratio, as seen in the central colourbar, with darker (and larger) dots depicting galaxies with a higher value of M*/Mtot, i.e., with less DM.
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