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Toward Resolution Convergence for Star Formation and Galactic Winds in Galaxy Simulations
The predictive power of hydrodynamic simulations of galaxies is often hampered by the resolution dependence of sub-grid models for star formation (SF) and stellar feedback. We present three-dimensional hydrodynamic simulations of an M82-like low-mass starburst galaxy at resolutions of 4, 8, 16, 32 p
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