Fig. 7
Stellar mass density distribution in galaxies with stellar masses > 1010.2 M⊙ of the composite cluster as a function of radial distance. Comparing these distributions to those shown in Fig. 6, we find that the stellar mass distributions are peaked more strongly than the number density distribution. That is an indication for mass segregation of quiescent galaxies in these systems. The lower panel shows the fraction of stellar mass in galaxies with a spectroscopic redshift.
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