Fig. 6.
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Evolution of the GC orbital semi-major and eccentricity during the whole backward integration time in the case of 411321 TNG-TVP. The inner GCs (a ≤ 3 kpc) have more regular and larger eccentricity changes during the evolution. The outer GCs (a > 3 kpc) have much smaller eccentricity changes during the whole backward integration time.
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