Star-forming gas clouds are strongly magnetized, and their ionization fractions are high
enough to place them close to the regime of ideal magnetohydrodyamics on all but the …

We use three-dimensional hydrodynamic simulations of vertically stratified patches of
galactic discs to study how the spatio-temporal clustering of supernovae (SNe) enhances …

Context. Young massive stellar clusters are extreme environments and potentially provide
the means for efficient particle acceleration. Indeed, they are increasingly considered as …

We revisit the problem of the growth of dense/cold gas in the cloud-crushing set-up with
radiative cooling. The relative motion between the dense cloud and the diffuse medium …

We compute the production of cosmic rays (CRs) in the dynamical superbubble (SB)
produced by a cluster of massive stars. Stellar winds, supernova remnants, and turbulence …

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 …

Context. Stellar feedback is a key contributor to the morphology and dynamics of the
interstellar medium in star-forming galaxies. In particular, energy and momentum input from …

Context. Star formation and stellar feedback are interlinked processes that redistribute
energy, turbulence, and material throughout galaxies. Because young and massive stars …

We critically assess limits on the maximum energy of protons accelerated within
superbubbles around massive stellar clusters, considering a number of different scenarios …

We use spherically symmetric hydrodynamic simulations to study the dynamical evolution
and internal structure of superbubbles (SBs) driven by clustered supernovae (SNe), focusing …