HD 1–0 and HD 2–1 integrated fluxes (calculated at 140 pc) for the models described in Sect. 2.4. The different colours indicate different disk masses. The observations for TW Hya are shown in black (Bergin et al. 2013; Kama et al. 2016b; D. Fedele, priv. comm.). The bottom right corner shows the region around the observations, where the shaded regions link models that are within the same mass bin.
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