Galaxy evolution is an important topic, and our physical understanding must be complete to
establish a correct picture. This includes a thorough treatment of feedback. The effects of …

Magnetic fields are fundamental to the evolution of galaxies, playing a key role in the
astrophysics of the interstellar medium and star formation. Large-scale ordered magnetic …

To what extent magnetic fields affect how molecular clouds (MCs) fragment and create
dense structures is an open question. We present a numerical study of cloud fragmentation …

We present the analysis of the magnetic field (B-field) structure of galaxies measured with far-
infrared (FIR) and radio (3 and 6 cm) polarimetric observations. We use the first data release …

Understanding the physical processes that regulate star formation and galaxy evolution are
major areas of activity in modern astrophysics. Nearby galaxies offer unique opportunities to …

Plain language summary The paper aims to demonstrate the need for a new large aperture
(50 m), single-antenna telescope receiving sub-millimeter and millimeter (hereafter sub-mm) …

As we learn more about the multi-scale interstellar medium (ISM) of our Galaxy, we develop
a greater understanding for the complex relationships between the large-scale diffuse gas …

We propose and apply a method to quantify the morphology of the large-scale ordered
magnetic fields (B-fields) in galaxies. This method is adapted from the analysis of Event …

Context. Magnetic turbulence is classified as weak or strong based on the relative amplitude
of the magnetic field fluctuations compared to the mean field. These two classes have …

We use high-resolution magnetohydrodynamic simulations of isolated disc galaxies to
investigate the co-evolution of magnetic fields with a self-regulated, star-forming interstellar …