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Fig. 4.

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Velocity channel maps of 12CO(1–0) (a), 13CO(1–0) (b) and C18O(1–0) (c) toward W5. The emission has been integrated over 3.3 km s−1 around the local standard of rest velocities indicated in each panel. Note: the intensity of each detected and displayed pixel is greater than 3σ. For the yellow stars and small green and red dots, see Fig. 2.

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