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Fig. 6

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2D temperature structure and dust temperature at ALMA surfaces for different values of amax. Top: 2D temperature structure of the fiducial active disk. The light green lines denote the height where the vertical extinction optical depth reaches unity at ALMA Bands 4 (solid), 6 (dashed), 7 (dash-dotted), and 8 (dotted). Bottom: Dust temperature at the height where the vertical extinction optical depth at the ALMA wavelengths reaches unity. The radial profile are not beam-convolved. The dust settling is not taken into account. The dust is assumed to be compact with a size distribution of pd = 3.5. The dust surface density is set so that τ10,B4 = 3.

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