In the G34.43+0.24 infrared dark cloud, radiative torque alignment explains the polarization hole except toward the hot cores, where radiation-driven grain disruption may reduce polarization.
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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
In the G34.43+0.24 infrared dark cloud, radiative torque alignment explains the polarization hole except toward the hot cores, where radiation-driven grain disruption may reduce polarization.