The star formation rate (SFR) in galactic disks depends on both the quantity of the available
interstellar medium (ISM) gas and its physical state. Conversely, the ISM's physical state …

Large-scale outflows in star-forming galaxies are observed to be ubiquitous and are a key
aspect of theoretical modeling of galactic evolution, the focus of the Simulating Multiscale …

We present the fourth simulation of the Cholla Galactic OutfLow Simulations suite. Using a
physically motivated prescription for clustered supernova feedback, we successfully drive a …

Astrophysical gases are commonly multiphase and highly turbulent. In this work, we
investigate the survival and growth of cold gas in such a turbulent, multiphase medium using …

Massive, young stars are the main source of energy that maintains multiphase structure and
turbulence in the interstellar medium (ISM), and without this" feedback" the star formation …

We study the propagation of mildly relativistic cosmic rays (CRs) in multiphase interstellar
medium environments with conditions typical of nearby disk galaxies. We employ the …

Cosmic rays (CRs) are an important component in the interstellar medium, but their effect on
the dynamics of the disc–halo interface (< 10 kpc from the disc) is still unclear. We study the …

We present the most sensitive and detailed view of the neutral hydrogen () emission
associated with the Small Magellanic Cloud (SMC), through the combination of data from the …

We present the first results from a high-resolution simulation with a focus on galactic wind
driving for an isolated galaxy with a halo mass of∼ 10 11 M⊙(similar to the Large …

Pressure balance plays a central role in models of the interstellar medium (ISM), but whether
and how pressure balance is realized in a realistic multiphase ISM is not yet well …