Understanding the physical mechanisms that control galaxy formation is a fundamental
challenge in contemporary astrophysics. Recent advances in the field of astrophysical …

Spiral galaxies, including the Milky Way, have large-scale magnetic fields with significant
energy densities. The dominant theory attributes these magnetic fields to a large-scale …

The physics of magnetic fields (B) and cosmic rays (CRs) have recently been included in
simulations of galaxy formation. However, significant uncertainties remain in how these …

Synchrotron emission is one of few observable tracers of galactic magnetic fields (B) and
cosmic rays (CRs). Much of our understanding of B in galaxies comes from utilizing …

We present the first data release of the Survey on extragALactic magnetiSm with SOFIA
(SALSA Legacy Program) with a set of 14 nearby (< 20 Mpc) galaxies with resolved imaging …

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 …

Galaxies are observed to host magnetic fields with a typical total strength of around 15 μ G.
A coherent large-scale field constitutes up to a few microgauss of the total, while the rest is …

Despite their ubiquity, there are many open questions regarding galactic and cosmic
magnetic fields. Specifically, current observational constraints cannot rule out whether …

The interstellar medium in the Milky Way's Central Molecular Zone (CMZ) is known to be
strongly magnetised, but its large-scale morphology and impact on the gas dynamics are not …

The magnetic fields in our Milky Way can be revealed by the distribution of Faraday rotation
measures (RMs) of radio sources behind the Galaxy and of radio pulsars inside the Galaxy …