Planck intermediate results - XXXIII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps

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Fig. 4

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Same as Fig. 1 for part of the Taurus molecular cloud around the B211 (north-west) and the L1506 (south-east) filaments. The numbers and white lines on the total intensity map correspond to the positions of the different cuts used to derive the radial profiles shown in Figs. 5 and 6.

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