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Fig. B.8


Distribution of the sample’s galaxies in the dynamical mass Mdyn vs. stellar mass M plane using the Sersic fit parameters. The alternative candidates are indicated by black stars. The galaxies belonging to the Ta10 sample are represented using filled green triangles, and the Tr09 sample is indicated by filled cyan diamonds. B19 is indicated by a filled grey square.The magenta dashed line marks the limiting scaling central velocity dispersion for our sample selection. The black dashed line denotes the limit of the Mdyn to M ratio, which is still considered to be physical, because M would exceed Mdyn above it.

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