Fig. D.3.
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Evolution of the stellar mass: Evolution of the total stellar mass of bound globular cluster particles, for each simulated cluster. Clusters originally embedded in a dark matter mini-halo (i.e. ⋆•) are displayed in green, while those devoid of the mini-halo (i.e. ⋆) are represented in red. Bound particles were defined according to Section 2.3.
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