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Fig. A.3.

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CO(3-2) spectra extracted using increasingly larger apertures from the primary-beam corrected ALMA and ACA data cubes. The channel widths are 21, 64, 86 km s−1 for the ALMA r = 1″, 2.5″, 4″ spectra (top panel), 86 km s−1 for the ALMA r = 7.5″ and 10″ spectra (middle panel), and 160 km s−1 for the ACA spectra (bottom panel). The aperture radii (or, in the case of elliptical apertures, the major and minor semi-axes) are reported on the plots. The top-right insets in each panel show the Gaussian spectral fits to the ALMA rap = 1″ (top), ALMA rap = 7.5″ (middle), and ACA rap = 15″ (bottom) spectra.

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