Magnetic Fields in Massive Star-forming Regions (MagMaR). IX. Radiative Torque Alignment and Disruption in NGC6334I

arXiv:2609.03458 · astro-ph.GA · Submitted 2026-09-03 · Read on arXiv

astro-ph.GA

Submitted: 2026-09-03

Updated: 2026-09-06

Code: https://github.com/gxli/volume-density-mapper

Terminology

• Alignment — 77× in this paper · explained in 1 episode
• Core — 30× in this paper · explained in 2 episodes
• Stellar Feedback — 3× in this paper · explained in 2 episodes
• Trace — 3× in this paper · explained in 2 episodes
• APEX — 2× in this paper · explained in 1 episode
• Anisotropy — 2× in this paper · explained in 3 episodes
• Degeneracy — 2× in this paper · explained in 3 episodes
• Korea Astronomy and Space Science Institute — 2× in this paper
• Abundance — 1× in this paper · explained in 1 episode
• Accuracy — 1× in this paper · explained in 1 episode
• Anti-correlation — 1× in this paper · explained in 3 episodes

Sources

• Optical and Magnetic Properties of Dust Grains
• Observations and Theory of Dynamical Triggers for Star Formation
• Magnetic fields in Massive Star-Forming Regions (MagMaR). VIII. Magnetic field overrun by gravity in GGD 27's accretion streamers
• Synthetic Modelling of Polarized Dust Emission in Intermediate-Mass YSOs: I: Constraining the Role of Iron Inclusions and Inelastic Relaxation on Grain Alignment with ALMA Polarization
• SIMPLIFI-Study of Interstellar Magnetic Polarization: A Legacy Investigation of Filaments. II. Enhancement of grain alignment near embedded protostars in the DR21 Ridge
• Volume Density Mapper: 3D Density Reconstruction Algorithm for Molecular Clouds
• The dominance of turbulence over magnetism in the formation of massive star cluster seeds
• Ne and Fe abundances in the ISM: Archival Study of Fe-L and Ne-K edges in Chandra and XMM-Newton
• Magnetic fields in star formation: from clouds to cores
• B-fields And dust in interstelLar fiLAments using Dust POLarization (BALLAD-POL): VI. Grain alignment mechanisms in the massive quiescent filament G16.96+0.27 using dust polarization observations from JCMT/POL-2
• Magnetic Fields in Massive Star-forming Regions (MagMaR). VII. On the dynamical importance of B-fields in massive protocluster W33 A

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