Gravity Driven Magnetic Field at ~1000 au Scales in High-mass Star Formation
Patricio Sanhueza, Josep Miquel Girart, Marco Padovani, Daniele Galli,, Charles L. H. Hull, Qizhou Zhang, Paulo Cortes, Ian W. Stephens, Manuel, Fernandez-Lopez, James M. Jackson, Pau Frau, Patrick M. Kock, Benjamin Wu,, Luis A. Zapata, Fernando Olguin, Xing Lu, Andrea Silva

TL;DR
This study uses high-resolution ALMA observations to analyze magnetic fields in a high-mass star-forming region, revealing a weakly magnetized environment where gravity dominates over other forces.
Contribution
It provides the first detailed magnetic field morphology and strength measurements at ~700 au scales in a high-mass star-forming core, highlighting gravity's dominance.
Findings
Magnetic field is weakly magnetized with a mass-to-flux ratio of 8.38.
Magnetic field morphology shows spiral-like, whirlpool features.
Gravity overwhelms turbulence, rotation, and magnetic forces at observed scales.
Abstract
A full understanding of high-mass star formation requires the study of one of the most elusive components of the energy balance in the interstellar medium: magnetic fields. We report ALMA 1.2 mm, high-resolution (700 au) dust polarization and molecular line observations of the rotating hot molecular core embedded in the high-mass star-forming region IRAS 18089-1732. The dust continuum emission and magnetic field morphology present spiral-like features resembling a whirlpool. The velocity field traced by the H13CO+ (J=3-2) transition line reveals a complex structure with spiral filaments that are likely infalling and rotating, dragging the field with them. We have modeled the magnetic field and find that the best model corresponds to a weakly magnetized core with a mass-to-magnetic-flux ratio (lambda) of 8.38. The modeled magnetic field is dominated by a poloidal component, but with an…
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