Fig. 5.
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Stacked radial profiles of the ex situ stellar mass fraction for 10 000 MaNGA galaxies as predicted from the diffusion model. (a) The median of the stacked radial profiles separated in 3 stellar mass bins. (b) The median of the stacked radial profiles in each group, following the classification based on the central ex situ gradient. The shaded regions enclose 68% of all data.
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