Magnetic fields are now widely recognized as critical at many scales to galactic dynamics
and structure, including multiphase pressure balance, dust processing, and star formation …

Magnetic fields grow quickly, even at early cosmological times, suggesting the action of a
small-scale dynamo (SSD) in the interstellar medium (ISM) of galaxies. Many studies have …

Quantifying the efficiency of dust destruction in the interstellar medium (ISM) due to
supernovae (SNe) is crucial for the understanding of galactic dust evolution. We present 3D …

Stratified discs with strong horizontal magnetic fields, are susceptible to magnetic buoyancy
instability (MBI). Modifying the magnetic field and gas distributions, this can play an …

Magnetic fields grow quickly even at early cosmological times, suggesting the action of a
small-scale dynamo (SSD) in the interstellar medium of galaxies. Many studies have …

We study the linear properties, non-linear saturation, and a steady, strongly non-linear state
of the Parker instability in galaxies. We consider magnetic buoyancy and its consequences …

Pseudodisks are dense structures formed perpendicular to the direction of the magnetic field
during the gravitational collapse of a molecular cloud core. Numerical simulations of the …

Dust in the interstellar medium (ISM) is critical to the absorption and intensity of emission
profiles used widely in astronomical observations, and necessary for star and planet …

The deposition of energy and momentum by supernova explosions has been subject to
numerous studies in the past few decades. However, while there has been some work that …

Recent observations have revealed a gallery of substructures in the dust component of
nearby protoplanetary discs, including rings, gaps, spiral arms, and lopsided concentrations …