We present simulations of the multiphase interstellar medium (ISM) at solar neighbourhood
conditions including thermal and non-thermal ISM processes, star cluster formation, and …

Star formation is a fundamental process for galactic evolution. One issue over the last
several decades has been determining whether star formation is induced by external …

Synthetic observations are playing an increasingly important role across astrophysics, both
for interpreting real observations and also for making meaningful predictions from models. In …

Radiation transport plays a crucial role in star formation models, as certain questions within
this field cannot be accurately addressed without taking it into account. Given the high …

We present a novel set of stellar feedback models, implemented in the moving-mesh code
arepo, designed for galaxy formation simulations with near-parsec (or better) resolution …

Supernovae (SNe) dominate the energy and momentum budget of stellar feedback, but the
efficiency with which they couple to the interstellar medium (ISM) depends strongly on how …

We describe a population of young star clusters (SCs) formed in a hydrodynamical
simulation of a gas-rich dwarf galaxy merger resolved with individual massive stars at …

Aims. We present the first simulations of the formation and feedback of massive stars which
account for radiation forces as well as photoionization feedback (along with protostellar …

We present high-resolution hydrodynamical simulations of isolated dwarf galaxies including
self-gravity, non-equilibrium cooling and chemistry, interstellar radiation fields (ISRF) and …

The first stars, galaxies, star clusters, and direct-collapse black holes are expected to have
formed in low-mass (∼ 105–109 M⊙) haloes at Cosmic Dawn (z∼ 10–30) under conditions …