Table 3.
Parameters of the disk + wind models of Hönig & Kishimoto (2017).
| Parameter | Symbol | Uniform prior | Posterior percentiles | ||
|---|---|---|---|---|---|
| 16 | 50 | 84 | |||
| Radial distribution power law index disk(ra) | a | [−3.0,−0.5] | −1.8 | −1.7 | −1.5 |
| Number of clouds along an equatorial ray | N0 | [5,10] | 6 | 8 | 9 |
| Scale height of the disc | h | [0.1,0.5] | 0.13 | 0.17 | 0.22 |
| Radial distribution power law index wind (ra) | aw | [−2.5,−0.5] | −0.8 | −0.7 | −0.6 |
| Half-opening angle of the wind | θw | [30°,45°] | 37° | 40° | 43° |
| Angular width of the hollow wind cone | σ | [7°,15°] | 10° | 12° | 14° |
| Wind-to-diskratio of dust clouds | fwd | [0.15,2.25] | 1.5 | 1.8 | 2.1 |
| Outer radius | rout | [450,500] | 471 | 484 | 494 |
| Inclination | i | [0°,90°] | 7° | 13° | 20° |
| Foreground extinction (mag) | AV | [0,2] | 0.2 | 0.5 | 1.0 |
| Covering factor | CT | ... | 0.49 | 0.66 | 0.82 |
| Type-2 probability | 1-Pesc | ... | 0.00 | 0.12 | 0.95 |
| Torus extinction (mag) | AVLOS | ... | 0.01 | 7 | 160 |
Notes. i = 0 is face-on and i = 90 is edge-on. The optical depth per cloud is τV = 50, and AV is defined as treated as in Table 2. These models use a mixture of the standard ISM dust composition of 53% silicates and 47% graphites with maximum sizes of 1 μm in the disc, plus a graphite-dominated population of small grains (sizes ≤ 0.25 μm), and large graphites only in the wind (0.75–1 μm). CT, Pesc, and
as in Table 2, but with
.
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