Understanding the physical mechanisms that control galaxy formation is a fundamental
challenge in contemporary astrophysics. Recent advances in the field of astrophysical …

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 …

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

Abstract The SILCC (SImulating the Life-Cycle of molecular Clouds) project aims to self-
consistently understand the small-scale structure of the interstellar medium (ISM) and its link …

We study the impact of stellar winds and supernovae on the multiphase interstellar medium
using three-dimensional hydrodynamical simulations carried out with flash. The selected …

We investigate the early impact of single and binary supernova (SN) explosions on dense
gas clouds with three-dimensional, high-resolution, hydrodynamic simulations. The effect of …

Understanding the physical processes that govern the dynamical behavior of the interstellar
medium (ISM) is central to much of modern astronomy and astrophysics. The ISM is the …

Context. The Orion Molecular Cloud is the nearest massive-star forming region. Massive
stars have profound effects on their environment due to their strong radiation fields and …

We use hydrodynamical simulations in a (256 pc) 3 periodic box to model the impact of
supernova (SN) explosions on the multiphase interstellar medium (ISM) for initial densities …

Photoionizing radiation and stellar winds from massive stars deposit energy and momentum
into the interstellar medium (ISM). They might disperse the local ISM, change its turbulent …