2 papers
astro-ph.GA2026
The dominance of turbulence over magnetism in the formation of massive star cluster seeds
Junhao Liu, Patricio Sanhueza, Piyali Saha +32
High-mass stars form in protoclusters, where gravo-magnetic processes shape collapsing clouds and clumps to be elongated preferentially perpendicular to magnetic (B) fields. Yet it…
astro-ph.GA2024
Applying the Velocity Gradient Technique in NGC 1333: Comparison with Dust Polarization Observations
Archana Soam, Ka Ho Yuen, Ian Stephens +3
Magnetic fields (B-fields) are ubiquitous in the interstellar medium (ISM), and they play an essential role in the formation of molecular clouds and subsequent star formation. Howe…