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Fig. A.1.

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[C I] 609 μm line profile toward d203-506 and the two-component Gaussian fit. The velocity centroid difference of the two components is 2.3 ± 0.4 km s−1 and suggests that the blueshifted emission arises from a slow wind not seen in HCO+ 4–3 emission (see Fig. 2).

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