Star formation lies at the center of a web of processes that drive cosmic evolution:
generation of radiant energy, synthesis of elements, formation of planets, and development …

Over the last decade block-structured adaptive mesh refinement (SAMR) has found
increasing use in large, publicly available codes and frameworks. SAMR frameworks have …

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

The enormous radiative and mechanical luminosities of massive stars impact a vast range of
scales and processes, from the reionization of the universe, to the evolution of galaxies, to …

We present a set of three-dimensional, radiation-magnetohydrodynamic calculations of the
gravitational collapse of massive (300 M☉), star-forming molecular cloud cores. We show …

Stellar feedback in the form of radiation pressure and magnetically driven collimated
outflows may limit the maximum mass that a star can achieve and affect the star formation …

The star-forming efficiency of dense gas is thought to be set within cores by outflow and
radiative feedback. We use magnetohydrodynamic simulations to investigate the relation …

Young massive star clusters inhabit regions of star formation and play an essential role in
the galactic evolution. They are sources of both thermal and non-thermal radiation, and are …

The protostellar outflows of wide-separation forming binaries frequently appear misaligned.
We use magneto-hydrodynamic simulations to investigate the alignment of protostellar spin …

Star formation is a multi-scale, multi-physics problem ranging from the size scale of
molecular clouds (∼ 10 ∼10 s pc) down to the size scales of dense prestellar cores (∼ 0.1 …