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Fig. 1

image

Gas (Σg, solid lines) and dust (Σd, dashed lines) surface densities for the inner 180 au of our fiducial disk models. Top panel: initial SMOOTH model without any gaps or rings. The grey star symbol indicates the gas surface density of 44.4 g cm−2 as measured by Booth et al. (2019) using 13C17O J = 3−2 observationswith a spatial resolution of ≈70 au. Bottom panel: models using the same fitted dust surface density profile but varying gas surface density profiles (see Sect. 2.4). All models are described in Table 1.

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