Globular clusters are dense, ancient groupings of stars that have survived the long history of galaxy formation and evolution, yet the exact processes that shape them from birth to the present day remain unclear. Here, we present AuriGLOBES (Auriga GLOBular clustEr Simulations), a new physical model designed to track how star clusters form and evolve within large-scale cosmological simulations. Using this model, we simulated nine galaxies similar in mass to the Milky Way and five lower-mass galaxies. Our simulations successfully produce realistic globular cluster systems that match
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