Calibrated, cosmological hydrodynamical simulations with variable IMFs III: Spatially-resolved properties and evolution

no code implementations • 30 Jul 2018 • Christopher Barber, Joop Schaye, Robert A. Crain

We find negative metallicity radial gradients for both simulations, but positive and flat [Mg/Fe] gradients in LoM-50 and HiM-50, respectively.

Astrophysics of Galaxies