Fig. A.1
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Continuum fluxes at λ = 0.89 mm and sizes of our disc models compared to class 0/I discs from the Orion star forming region. Solid lines show model mod-a-3-r40 and dashed lines model mod-a-2-r10. Similar to the eDisk sample shown in Fig. 4 and Fig. 5, the model with less efficient viscous heating and higher angular momentum agrees better with the observed sample.
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