Open Access

Fig. C.14


Same as Fig. C.4 for SerpS-MM18. The PG model is the best-fit model to reproduce the 231 GHz visibility profile: it includes a marginally resolved additional Gaussian component with an FWHM 0.13′′ (flux 76 mJy). The 94 GHz profile can be well modeled with a Plummer-only envelope model.

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