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Fig. 7


Size-luminosity relation. Symbols as in Fig. 2 including the dSphs from the Milky Way (grey triangles) and M31 (grey squares). The blue line in the V band is the fit by Shen et al. (2003) for late-type galaxies. The dotted dashed line is the fit for dSphs by Brasseur et al. (2011). All the half light radii have been transformed to semi-major radii, but the fit (solid line) and 1σ scatter (dotted lines) for the SAURON early-type galaxies from FB11 is based on geometric radii.

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