Apostle–Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
Apostle–Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
Modern hydrodynamical simulations reproduce many properties of the real universe. These simulations model various physical processes, but many of these are included using `subgrid models' due to resolution limits. Although different subgrid models have been successful in modelling the effects of supernovae (SNe) feedback on galactic properties, it remains unclear …