Abstract The Polarisation Sky Survey of the Universe's Magnetism (POSSUM) will conduct a
sensitive∼ 1 GHz radio polarization survey covering 20,000 deg 2 of the southern sky with …

Abstract We present new 13 CO (1− 0), C 18 O (1− 0), HCO+(1− 0), and H 13 CO+(1− 0)
maps from the IRAM 30 m telescope and a spectrally resolved [C ii] 158 μm map observed …

To investigate the role of magnetic fields in the evolution of the interstellar medium,
formation and evolution of molecular clouds, and ultimately the formation of stars, their three …

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 …

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 …

We study the H ii regions associated with the NGC 6334 molecular cloud observed in the
submillimeter and taken as part of the B-fields In STar-forming Region Observations Survey …

We present evidence for scale-independent misalignment of interstellar dust filaments and
magnetic fields. We estimate the misalignment by comparing millimeter-wave dust …

Context. Ultra-high-energy cosmic rays (UHECRs) are highly energetic charged particles
with energies exceeding 10 18 eV. These energies are far greater than those achieved in …

The mapping of the Galactic magnetic field (GMF) in three dimensions is essential to
comprehend various astrophysical processes that occur within the Milky Way. This study …

We analyze the internal dynamics of young stars toward Perseus using Gaia EDR3 data,
including Per OB2 and California Cloud. Interpreting the current dynamics, we speculate that …