Star clusters stand at the intersection of much of modern astrophysics: the ISM, gravitational
dynamics, stellar evolution, and cosmology. Here, we review observations and theoretical …

We discuss some of the key open questions regarding the formation and evolution of
globular clusters (GCs) during galaxy formation and assembly within a cosmological …

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 …

Giant molecular clouds (GMCs) are the sites of star formation and stellar feedback in
galaxies. Their properties set the initial conditions for star formation and their lifecycles …

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 variability of galaxy star formation histories (SFHs) across a range of time-
scales provides insight into the underlying physical processes that regulate star formation …

The initial mass function (IMF) of stars is a key quantity affecting almost every field of
astrophysics, yet it remains unclear what physical mechanisms determine it. We present the …

We report the formation of bound star clusters in a sample of high-resolution cosmological
zoom-in simulations of z≥ 5 galaxies from the Feedback In Realistic Environments project …

We present the first simulations evolving resolved spectra of cosmic rays (CRs) from MeV–
TeV energies (including electrons, positrons,(anti) protons, and heavier nuclei), in live …

Radiative feedback (RFB) from stars plays a key role in galaxies, but remains poorly
understood. We explore this using high-resolution, multifrequency radiation-hydrodynamics …