Fig. 20
For a sample of galaxies in the Virgo cluster (taken from Kormendy et al. 2009) we plot the position on the major axis (in arcsec) to which they can be resolved into individual stars using MICADO/MAORY at two different surface brightness limits (SB). The same sample of galaxies is plotted in each case; 10 dwarf spheroidals (in red); 27 elliptical galaxies (black) and 5 S0 galaxies (blue).
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