B-fields And dust in interstelLar fiLAments using Dust POLarization (BALLAD-POL): III. Grain alignment and disruption mechanisms in G34.43+0.24 using polarization observations from JCMT/POL-2
Saikhom Pravash, Archana Soam, Pham Ngoc Diep, Thiem Hoang, Nguyen, Bich Ngoc, Le Ngoc Tram

TL;DR
This study investigates grain alignment and disruption mechanisms in a filamentary molecular cloud using polarization observations, revealing the roles of magnetic field tangling and radiative torques in polarization features.
Contribution
It provides new insights into grain alignment and disruption processes in G34.43+0.24, especially highlighting the effects of magnetic field tangling and radiative torques in different regions.
Findings
Polarization fraction decreases with increasing intensity and density.
Magnetic field tangling significantly causes depolarization in South region.
RAT alignment explains polarization in North and Center regions, with evidence of RAT-D in cores.
Abstract
Polarization of starlight and thermal dust emission due to aligned non-spherical grains helps us to trace magnetic field (B-field) morphology in molecular clouds and to study grain alignment mechanisms. In this work, we study grain alignment and disruption mechanisms in a filamentary infrared dark cloud G34.43+0.24 using thermal dust polarization observations from JCMT/POL-2 at 850 . We study in three sub-regions as North harboring MM3 core, Center harboring MM1 and MM2 cores and South having no core. We find the decrease in polarization fraction P with increasing total intensity and gas column density, known as polarization hole. To disentangle the effect of magnetic field tangling on the polarization hole, we estimate the polarization angle dispersion function. We find depolarizations in North and Center regions are due to decrease in net alignment efficiency of grains…
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Taxonomy
TopicsAtmospheric Ozone and Climate · Ionosphere and magnetosphere dynamics · Geophysics and Gravity Measurements
