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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°] 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 A V LOS $ \mathrm{A}_{\mathrm{V}}^{\mathrm{LOS}} $ as in Table 2, but with N LOS ( i ) = N 0 f wd e ( ( 90 i ) θ w ) 2 / 2 σ 2 + N 0 e ( tan ( 90 i ) ) 2 / 2 h 2 $ \mathrm{N}_{\mathrm{LOS}}(\mathrm{i}) = \mathrm{N}_0\ \mathrm{f}_{\mathrm{wd}}\ \mathrm{e}^{-((90-\mathrm{i})-\theta_{\mathrm{w}})^2/2 \sigma^2} + \mathrm{N}_0\ \mathrm{e}^{-(\mathrm{tan}(90-\mathrm{i}))^2/2 \mathrm{h}^2} $.

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