Fig. 1

Integrated absolute V magnitude vs. the logarithm of the half-light radius for dwarf galaxies in the most recent version of the M12 catalogue (filled circles). The mean MV vs. log Rh relation by Brasseur et al. (2011) is plotted as a continuous line; the curves bracketing ± 1σ and ± 2σ range about that relation are plotted as dashed and dotted lines, respectively. The middle, unshaded area of the figure highlights the range of MV considered here. Large empty circles indicate the synthetic dwarf galaxies under study (see also Fig. 2).
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