Fig. 6
Color–magnitude diagram (U − V) − MV for Abell 1795 (this work) and for Abell 754 (McIntosh et al. 2005). The straight lines in the plots correspond to the best-fit parameters given for Abell 754 in Table 8 of McIntosh et al. (2005) last row. The red and green dots in the upper panel, respectively mark elliptical and S0 galaxies that are spectroscopically confirmed members of the cluster Abell 1795.
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