The role of accreted and in situ populations in shaping the stellar halos of low-mass galaxies

Open Access

Fig. B.1.

[Fe/H] distributions of the in situ (blue) and accreted (orange) components of the stellar halo, normalised by the number of particles of each population. We also show the overall [Fe/H] distribution of the stellar halo colour-coded by the accreted mass of the stellar halo.

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