The distribution of globular clusters in kinematic spaces does not trace the accretion history of the host galaxy

Open Access

Fig. A.3.

Distribution of GCs in the E − L_z space at the end of the simulations. Top panel: Distribution from the single-accretion simulation (MWsat_n1_Φ60). Bottom panel: Distribution from the double accretion simulation (MWsat_n2_Φ30-150). The MW’s GCs are identified as grey circles, while satellite(s) GCs are represented as magenta and orange circles.

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