Observations that resolve nearby galaxies into individual regions across multiple phases of
the gas–star formation feedback “matter cycle” have provided a sharp new view of molecular …

Recent discoveries of a significant population of bright galaxies at cosmic dawn $\left
(z\gtrsim 10\right) $ have enabled critical tests of cosmological galaxy formation models. In …

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 …

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 …

The star formation rate (SFR) in galactic disks depends on both the quantity of the available
interstellar medium (ISM) gas and its physical state. Conversely, the ISM's physical state …

We characterize mass, momentum, energy, and metal outflow rates of multiphase galactic
winds in a suite of FIRE-2 cosmological 'zoom-in'simulations from the Feedback in Realistic …

We introduce a suite of cosmological volume simulations to study the evolution of galaxies
as part of the Feedback in Realistic Environments project. FIREbox, the principal simulation …

One of the key mysteries of star formation is the origin of the stellar initial mass function
(IMF). The IMF is observed to be nearly universal in the Milky Way and its satellites, and …

Understanding the rate at which stars form is central to studies of galaxy formation.
Observationally, the star formation rates (SFRs) of galaxies are measured using the …

We use the FIRE-2 cosmological simulations to study the formation of a quasi-static, virial-
temperature gas phase in the circumgalactic medium (CGM) at redshifts 0< z< 5 and how …