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Table 5
Parameters of the best model.
| Parameter | Value |
|
|
|
| Dust species | Amorphous carbon |
| Grain size | 0.01 μm |
| Grain shape | Mie |
| Distance | 640 ± 190 pc |
| M ⋆ ⋆ | 1.1 ± 0.1 M⊙ |
... |
...0.4 ± 0.1 M⊙ |
... |
...0.7 ± 0.1 M⊙ |
| R in | 15 ± 1 AU |
| Rout/Rin | 2.2 ± 0.3 |
| M dust | (1.0 ± 0.4) × 10-8 M⊙ |
| p | 1.3 ± 0.3 |
| i | 60° ± 5° |
| PA | 130° ± 10° E of N |
|
|
|
|
12.1 |
|
2.3 |
|
0.2 |
|
1.9 |
|
0.2 |
Notes.
(a)
The primary and secondary mass are computed from M⋆ ⋆, the inclination of our best model, and the mass function of the primary star (see Sect. 7.5).
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