Image Details
Caption: Figure 16.
Middle and lower panels: scaling relations for early-type galaxies and globular clusters (GCs) in the Virgo cluster, Fornax cluster, and Local Group (see the text for details). For galaxies in Fornax and the Local Group, apparent B-band magnitudes and effective radii in arcseconds have been calculated as they would appear at the distance of the Virgo cluster. The dotted and dashed lines indicate the approximate selection limits for the Virgo survey of Binggeli et al. (1985) and the NGVS, respectively. The regions of parameter space where galaxies or star clusters in Virgo would be resolved are labeled, assuming an NGVS resolution limit of R e = 10 pc for compact sources (Section 5.1.4). The completeness function for the galaxy sample shown here is given in the top panel. The yellow star identifies the location of the galaxy shown in Figure 17.
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