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Fig. 9.

image

Projected radial distribution of the metallicity of the GCs relative to the host metallicity taken from Iodice et al. (2019a), i.e. [M/H]GC–[M/H]gal, colour-coded by the (gz) colour (left) and by the host stellar mass (right). The black line indicates an offset of zero dex and the dotted lines give the typical scatter found in the host metallicities of ±0.1 dex. There are less GCs shown than in Fig. 8 because not all F3D galaxies have metallicity maps available.

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