Fig. 2.
Stellar fraction as a function of the stellar mass for simulated centrals in EAGLE (left panel) and IllustrisTNG (right panel) with M⋆ > 5 × 1010 M⊙, compared to nearby spirals from the SPARC dataset (red circles with error bar). Coloured symbols are used for our sub-sample of simulated discs. The purple shaded region shows the AM relation and related scatter from Moster et al. (2013).
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