A new classification of ex situ and in situ Galactic globular clusters based on a method trained on Milky Way analogues in the TNG50 cosmological simulations

Open Access

Fig. 9

Coherence loss in energy: probability density P(σ_E) of the energy dispersion for our ex situ GCs in the 198 MW analogues at z=0. We calculate the energy dispersions for each ex situ GC groups. The evolution of the galactic potential induces a greater energy dispersion for GCs originating from the same satellite.

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