We present the S-Band Polarization All Sky Survey (S-PASS), a survey of polarized radio
emission over the southern sky at Dec.<− 1° taken with the Parkes radio telescope at 2.3 …

Magnetic fields in the ionized medium of the disk and halo of the Milky Way impose Faraday
rotation on linearly polarized radio emission. We compare two surveys mapping the Galactic …

Faraday rotation occurs along every line of sight in the Galaxy; rotation measure (RM)
synthesis allows a 3D representation of the interstellar magnetic field. This study uses data …

We present the identification of the previously unnoticed physical association between the
Corona Australis molecular cloud (CrA), traced by interstellar dust emission, and two shell …

Neutral hydrogen (H i) bubbles and shells are common in the interstellar medium (ISM).
Studying their properties provides insight into the characteristics of the local ISM as well as …

Context. Magnetic fields in the turbulent interstellar medium (ISM) are a key element in
understanding Galactic dynamics, but there are many observational challenges. One useful …

ABSTRACT Using the Global Magneto-Ionic Medium Survey (GMIMS) Low-Band South
(LBS) southern sky polarization survey, covering 300–480 MHz at 81 arcmin resolution, we …

Context. Faraday tomography of broadband radio polarization surveys enables us to study
magnetic fields and their interaction with the interstellar medium (ISM). Such surveys include …

There is a vitally important yet understudied aspect of astrophysics, one that works on large
and small scales, regulating star-formation, tracing galaxy mergers and interactions …