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

To better understand the nature of the multiphase material found in outflowing galaxies, we
study the evolution of cold clouds embedded in flows of hot and fast material. Using a suite …

We measure the net energy efficiency of supernova (SN) and stellar wind feedback in the
starburst galaxy M82 and the degree of mass loading of the hot gas piston driving its …

Motivated by observations of multiphase galaxy outflows, we explore the impact of isotropic
and anisotropic electron thermal conduction on the evolution of radiatively cooled, cold …

We have performed a series of three-dimensional simulations of the interaction of a
supersonic wind with a nonspherical radiative cloud. These simulations are motivated by our …

We have performed a series of three-dimensional simulations of a starburst-driven wind in
an inhomogeneous interstellar medium. The introduction of an inhomogeneous disk leads to …

Filamentary structures are ubiquitous in the interstellar medium, yet their formation, internal
structure, and longevity have not been studied in detail. We report the results from a …

We present a set of numerical experiments designed to systematically investigate how
turbulence and magnetic fields influence the morphology, energetics, and dynamics of …

Recent observations suggest that dense gas clouds can survive even in hot galactic winds.
Here we show that the inclusion of turbulent densities with different statistical properties has …

Ubiquitous detections of cold/warm gas around galaxies indicate that the circumgalactic
medium (CGM) is multiphase and dynamic. Recent state-of-the-art cosmological galaxy …