Fig. 3

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Map of polarization segments (rotated by 90°) and polarized intensity P (greyscale) in the NE1-NE2 filament in the high-mass star-forming region G327.7: observations (purple), from Beuther et al. (2020); best-fit model (green). The black contours show the observed 1.3 mm dust emission intensity starting from 3σ in steps of 6σ.
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