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

Open Access

Fig. 8.

Final GC distributions in the kinematic spaces E − L_z, L_perp − L_z, eccentricity − L_z, and the action space for the simulation MWsat_n2_Φ30-150. The in situ population of GCs is represented by grey circles, while the accreted populations are indicated with magenta for satellite 1 and orange for satellite 2.

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