Dust mass in protoplanetary disks with porous dust opacities

Open Access

Fig. 2

Comparison of F_1.3mm (upper panel) and T_dust (bottom panel) between models that use compact dust opacities (black) and porous dust opacities (blue), respectively. In the models, all of other parameters are fixed: R_c = 30 AU, Ψ = 1.15, H₁₀₀ = 10 AU.

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