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Table 5
Best-fit model setups for the inner disk.
| Model setup | Free parameters | ||||
|
|
|||||
| Dust setup | H out / r out | rout (au) | Mdust (M⊙) | p |
|
| 2 | 0.05 |
|
|
|
3.9 |
| 0.1 |
|
|
|
4.0 | |
| 5 | 0.03 |
|
|
|
4.4 |
| 0.05 |
|
|
|
4.0 | |
Notes. These best-fit model setups (with rin set to 0.2 au) fit the NIR data (
) equally. The quoted uncertainties are 1σ (68% confidence interval). The MIR data were not used here.
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