Stars do not generally form in isolation. Instead, they form in clusters, and in these clustered
environments, newborn stars can have profound effects on one another and on their parent …

I review the current state of numerical simulations of stellar feedback in the context of star
formation at scales ranging from the formation of individual stars to models of galaxy …

The role of turbulence and magnetic fields is studied for star formation in molecular clouds.
We derive and compare six theoretical models for the star formation rate (SFR)—the …

Compressible turbulence shapes the structure of the interstellar medium of our Galaxy and
likely plays an important role also during structure formation in the early Universe. The …

We present a smoothed particle hydrodynamics parameter study of the dynamical effect of
photoionization from O-type stars on star-forming clouds of a range of masses and sizes …

We present a census of molecular outflows across four active regions of star formation in the
Perseus molecular cloud (NGC 1333, IC348/HH211, L1448 and L1455), totalling an area of …

We investigate massive star formation in turbulent, magnetized, parsec-scale clumps of
molecular clouds including protostellar outflow feedback using three-dimensional numerical …

The physics of diffuse gas accretion and the properties of the cold and hot modes of
accretion on to proto-galaxies between z= 2 and 5.4 is investigated using the large …

Star formation is primarily controlled by the interplay between gravity, turbulence, and
magnetic fields. However, the turbulence and magnetic fields in molecular clouds near the …

Context. Even though turbulent motions are found everywhere in astrophysical systems, the
origin of this turbulence is poorly understood. When cosmic structures form, they grow in …