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We present the first results of a project aimed at following the formation and long‐term dynamical evolution of star clusters within the potential of a host galaxy. Here, we focus on a model evolved within a simplified potential representing the Large Magellanic Cloud. This demonstrates for the first time the self‐consistent formation of a bound star cluster from a giant molecular cloud. The model cluster reproduces the density profiles and structural characteristics of observed star clusters.

Self‐consistent simulations of star cluster formation from gas clouds under the influence of galaxy‐scale tidal fields