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Fig. 14


Polarisation vectors over-plotted on 0.4°×0.4° WISE 12 μm image of the field containing L673-7. The source L673-7-IRS is identified by a star. The molecular outflow direction is shown as a solid line with double arrow head. The broken line shows the direction of the Galactic plane at the latitude of the cloud. The vector with 2% polarisation is shown as reference. The positions of the SRAO observations are identified as circles A and B.

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