Galaxies and their dark-matter haloes have posed several challenges to the dark energy
plus cold dark matter (Λ CDM) cosmological model. These discrepancies between …

Neutral-atomic and molecular outflows are a common occurrence in galaxies, near and far.
They operate over the full extent of their galaxy hosts, from the innermost regions of galactic …

We introduce serra, a suite of zoom-in high-resolution (, at z= 7.7) cosmological simulations
including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post …

We analyse the first giant molecular cloud (GMC) simulation to follow the formation of
individual stars and their feedback from jets, radiation, winds, and supernovae, using the …

We describe a public data release of the FIRE-2 cosmological zoom-in simulations of galaxy
formation (available at http://flathub. flatironinstitute. org/fire) from the Feedback In Realistic …

As they grow, galaxies can transition from irregular/spheroidal with 'bursty'star formation
histories (SFHs), to discy with smooth SFHs. But even in simulations, the direct physical …

Increasingly, uncertainties in predictions from galaxy formation simulations (at sub-Milky
Way masses) are dominated by uncertainties in stellar evolution inputs. In this paper, we …

ABSTRACT We present STARFORGE (STAR FORmation in Gaseous Environments): a new
numerical framework for 3D radiation magnetohydrodynamic (MHD) simulations of star …

Recent observations of high-redshift galactic disks (z≈ 1–3) show a strong negative trend in
the dark-matter (DM) fraction f DM with increasing baryon surface density. For this to be true …

We present the escape fraction of hydrogen ionizing photons (f esc) from a sample of 34
high-resolution cosmological zoom-in simulations of galaxies at z≥ 5 in the Feedback in …