Fig. A.3
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Channel maps of the C18O (2−1) emission in GSS30 IRS3. Emission is detected above 5σ from −0.66 km s−1 to 5.19 km s−1. The color scale is stretched using the inverse hyperbolic sine function. The lowest contour emission corresponds to 5σ (1σ corresponds to 1.83 mJy beam−1), with increments of 10σ. The field of view of the map is 6″ × 6″.
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