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Consistent dust and gas models for protoplanetary disks I Disk shape, dust settling, opacities, and PAHs

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Figure

Fig. 2. Dust opacities used for the standard disk radiative transfer mod-and 15% amorphous carbon by volume
Fig. 3. Dust absorption coein brackets represent the log-log dust absorption opacity slopes between 0.85 mm and 1.3mm, and between 5 mm and 1 cm, see Appendixvolume fraction of amorphous carbon
Table 3. Model parameters, and values for the reference model.
Fig. 4. Summary of results from the reference model.(black) optical depthsorientations at 3 diand gas temperatures (in units of 10 K), the near-IR excess (in units of 0.05centre plot shows calculated line fluxes and full widths at half maximum (FWHM)
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