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Table 1
Distance from the star, temperature, and density conditions corresponding to midplane regions in the protoplanetary disk structure in Fig. 1, following the ProDiMo simulation of a passive irradiated disk (Woitke et al. 2009).
| r (AU) | T (K) | n ⟨ H ⟩ (cm-3) |
|
|
||
| 1 | 80 | 1014 |
| 3–4 | 65 | 1012 |
| 7–8 | 40 | 1011 |
| 10–15 | 20 | 1010 |
Notes. The stellar parameters used in this simulation are found in Table 2.
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