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We reproduced the orbital trajectories of 159 Globular Cluster subsystems in 10 Gyr lookback time using our own high-order N-body parallel dynamic code φ-GPU. Each Cluster was treated as a single physical particle assigned the position and velocity of the Globular Clusters center from the Gaia DR3 observations, according to Baumgardt.
To reproduce the dynamics of the Galaxy in time, we used five TNG-100 time-variable external potentials, which were selected from the large-scale cosmological database IllustrisTNG-100, and which in their characteristics (mass and size of disk and halo) are similar to the physical values of the Milky Way.
Below the list of Names with hyperlink for each Cluster, which orbital evolution reproduced and present in five TNG external potentials up 10 Gyr lookback time of cosmological scale.
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