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Table 5
Best-fit and deduced parameters found by optimization runs for the NIR images (A), SED data only (B), SED data only for the simple flared disk model with η = 1 (C), and mm-map/SED combined (D).
| Model | A | B | C | D |
|
|
||||
| η | 0.019 |
|
1 | 0.03 |
| α | 2.45 |
|
2.39 | 2.3 |
| β | 1.09 |
|
1.21 | 1.16 |
| p | 1.36 | 1.09 | 1.17 | 1.14 |
| Rin [AU] | 2.1 |
|
0.05 | 0.56 |
| Ratt [AU] | 59.6 |
|
na | 44.4 |
| Rout [AU] | 455 |
|
212 | 175 |
| h100 [AU] | 14.8 |
|
14.8 | 14.7 |
| mdust [10-5 M⊙] | 0.734 |
|
9.47 | 5.04 |
| min/mout | 0.09 | 0.11 | na | 0.15 |
| Teff [K] | 3200 |
|
4000 | 3300 |
| L ∗ [L⊙] | 0.6 |
|
0.38 | 0.48 |
| amin [μm] | 0.006 |
|
0.005 | 0.003 |
| amax [μm] | 1.87 |
|
7130 | 20 200 |
| d | 3.4 |
|
3.35 | 3.58 |
| i [°] | 83.6 |
|
80.1 | 85.1 |
|
|
||||
|
49 | 586 | 1079 | 781 |
|
8.2 × 107 | 12 884 | 59 130 | 41 471 |
|
17 7287 | 74 416 | 77 438 | 55 239 |
Notes. The confidence intervals of model B were deduced by the procedure described in Sect. 4.3 and are discussed in Sect. 5.2.
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