Multi-scale radiative-transfer model of the protoplanetary disc DoAr 44

Open Access

Fig. 6

$χ_{SED}^{2}$ $\$\chi_{\text {SED}}^{2}$$ contribution of the outer disc, for a variety of different particle sizes, from 100 nm to 100 μm. The curved low-density high-temperature sections correspond to optically thin solutions, and the vertical (isothermal) dark areas correspond to optically thick solutions.

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