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Fig. B.3.
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Final E − Lz distribution of GCs for the two simulations MWsat_n4_Φ150-60-0-30 (left panel) and MWsat_n4_Φ180-90-30-120 (right panel). GCs originating from the MW-type galaxy are identified as grey circles while accreted GCs are identified by colour-coded circles related to the different satellite of origin.
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