We summarize the results of a spectropolarimetric survey of 56 chemically peculiar (CP)
stars in the association of Orion OB1. We uniformly collected the observational material with …

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 …

Large-scale synchrotron loops are recognized as the main source of diffuse radio-continuum
emission in the Galaxy at intermediate and high Galactic latitudes, yet their origin remain …

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 …

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 report 850 μm continuum polarization observations toward the filamentary high-mass
star-forming region NGC 2264, taken as part of the B-fields In STar forming Regions …

The study of the development of structures on multiple scales in the cold interstellar medium
has experienced rapid expansion in the past decade, on both the observational and the …