THE IMPACT OF STAR FORMATION AND FEEDBACK RECIPES ON THE STELLAR MASS AND INTERSTELLAR MEDIUM OF HIGH-REDSHIFT GALAXIES
We introduce MEGATRON, a new galaxy formation model for cosmological radiation hydrodynamics simulations of high-redshift galaxies. The model accounts for the non-equilibrium chemistry and heating/cooling processes of ≥ 80 atoms, ions, and molecules, coupled to on-the-fly radiation transfer. We apply the model in a cosmological setting to the formation of a 109 M⊙halo at z = 6, and run 25 realizat
