We present a method to flexibly and self-consistently determine individual galaxies' star
formation rates (SFRs) from their host haloes' potential well depths, assembly histories, and …

ABSTRACT The Feedback In Realistic Environments (FIRE) project explores feedback in
cosmological galaxy formation simulations. Previous FIRE simulations used an identical …

Spectroscopic surveys of the Milky Way's stars have revealed spatial, chemical, and
kinematical structures that encode its history. In this work, we study their origins using a …

We study the implementation of mechanical feedback from supernovae (SNe) and stellar
mass loss in galaxy simulations, within the Feedback In Realistic Environments (FIRE) …

Quenched galaxies are often observed to contain a strong bulge component. The key
question is whether this reflects a causal connection–can star formation be quenched …

To improve our understanding of high-z galaxies, we study the impact of H2 chemistry on
their evolution, morphology and observed properties. We compare two zoom-in high …

We present a model that explains why galaxies form stars on a timescale significantly longer
than the timescales of processes governing the evolution of interstellar gas. We show that …

Numerical simulations have become one of the key tools used by theorists in all the fields of
astrophysics and cosmology. The development of modern tools that target the largest …

We present the results of a set of high-resolution chemo-dynamical simulations of dwarf
galaxies in a ΛCDM cosmology. Out of an original cosmological box, a sample of 27 systems …

The formation and evolution of stellar clusters is intimately linked to that of their host
galaxies. To study this connection, we present the emp-Pathfinder suite of cosmological …