Linearly polarized emission from dust grains and molecular spectroscopy is an effective
probe of the magnetic field topology in the interstellar medium and molecular clouds. The …

Context. A large-scale magnetic field permeates our Galaxy and is involved in a variety of
astrophysical processes, such as star formation and cosmic ray propagation. Dust …

Context. The magnetic field strength in interstellar clouds can be estimated indirectly from
measurements of dust polarization by assuming that turbulent kinetic energy is comparable …

The mean plane-of-sky magnetic field strength is traditionally obtained from the combination
of polarization and spectroscopic data using the Davis–Chandrasekhar–Fermi (DCF) …

Abstract The Davis–Chandrasekhar–Fermi (DCF) method provides an indirect way to
estimate the magnetic field strength from statistics of magnetic field orientations. We compile …

In a companion paper, we reported the self-consistent formation of quasar accretion disks
with inflow rates $\sim 10\,{\rm M_ {\odot}\, yr^{-1}} $ down to< 300 Schwarzschild radii from …

The relative role of turbulence, magnetic fields, and self-gravity in star formation is a subject
of intensive debate. We present IRAM 30 m telescope observations of the 13 CO (1–0) …

Cosmic rays (CRs) are a dynamically important component of the interstellar medium (ISM)
of galaxies. The∼ GeV CRs that carry most CR energy and pressure are likely confined by …

Turbulent gas motions are observed in the intracluster medium (ICM). The ICM is density-
stratified, with the gas density being highest at the centre of the cluster and decreasing …

Pulsars can act as an excellent probe of the Milky Way magnetic field. The average strength
of the Galactic magnetic field component parallel to the line of sight can be estimated as …