Formation of the Hub-Filament System G33.92+0.11: Local Interplay between Gravity, Velocity, and Magnetic Field
Jia-Wei Wang, Patrick M. Koch, Roberto Galv\'an-Madrid, Shih-Ping Lai,, Hauyu Baobab Liu, Sheng-Jun Lin, Kate Pattle

TL;DR
This study investigates the formation of a hub-filament system G33.92+0.11, revealing gravity's dominant role in shaping filaments and magnetic fields, with local interplay between gravity, velocity, and magnetic fields influencing star formation.
Contribution
It provides detailed observational analysis of filament, magnetic field, and velocity interactions in G33.92+0.11, highlighting gravity's primary influence in hub-filament system formation.
Findings
Filaments align with magnetic field and gravity in dense regions.
Velocity gradients are perpendicular to magnetic field and gravity in diffuse areas.
Gravity dominates over magnetic and kinetic energies in the system.
Abstract
The formation of filaments in molecular clouds is an important process in star formation. Hub-filament systems (HFSs) are a transition stage connecting parsec-scale filaments and proto-clusters. Understanding the origin of HFSs is crucial to reveal how star formation proceeds from clouds to cores. Here, we report JCMT POL-2 850 m polarization and IRAM 30-m CO (2-1) line observations toward the massive HFS G33.92+0.11. The 850 m continuum map reveals four major filaments converging to the center of G33.92+0.11 with numerous short filaments connecting to the major filaments at local intensity peaks. We estimate the local orientations of filaments, magnetic field, gravity, and velocity gradients from observations, and we examine their correlations based on their local properties. In the high-density areas, our analysis shows that the filaments tend to align with the…
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