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Fig. 9.

image

Distribution in M*,10 − Γ*,10 space of the galaxies in the SDSS sample, colour-coded by stellar velocity dispersion within an aperture of 10 kpc. The three bands mark 68% credible regions of values of the average stellar velocity dispersion, as inferred from the fit to the M*,10 − Γ*,10 fundamental plane (Eq. (5)).

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