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Fig. B.2


Top: emission at 250 μm and magnetic field toward the Musca (left) and IC 5146 (right) regions. The colors represent the emission observed in the Herschel 250 μm band. The draperypattern represents the magnetic field orientation averaged along the LOS and projected onto the plane of the sky, B, as inferred from the Planck 353 GHz data. Bottom: histograms of relative orientations for three representative column density bins.

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