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A new clump-based star formation model for galaxy simulations: implications for high-redshift compact star clusters
We develop a new star formation model for galaxy simulations in which star-forming gas clumps are identified on-the-fly and converted into stars with an efficiency $ε_{\rm SF}$ set by the clump surface density $Σ_{\rm c}$, calibrated against radiation hydrodynamics simulations of star cluster format
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