Table 4
Best-fit parameters resulting from SED and visibility fitting.
| Parameter | Literature value | Reference | Range explored | Best fit value |
|---|---|---|---|---|
| i | 60° | (1), (2) | 30–80° | 50° |
| Rinner | 0.18 | (1) (3) | 0.1–0.6 au | 0.15 au |
| Router | 100 au | (1) | 20.0–120.0 au | 100.0 au |
| h0 | ... | ... | 7.0–20.0 au | 15.0 au |
| αdisk | ... | ... | 1.0–3.0 | 2.4 |
| βdisk = (α − 1) | ... | ... | 0.0–2.0 | 1.4 |
| Dust:Gas | 0.01 | (1) | 0.01–0.008 | 0.01 |
| amin | 0.1 μm | (1) | 0.1–1.4 μm | 0.39 μm |
| qdist | 3.0 | (1) | 2.00–4.00 | 3.06 |
| Tsub | 1600 | (1) | 1400–2000 | 1600 K |
| Dusty disk wind parameter | Literature value | Reference | Range explored | Best fit value |
| R0min | ... | ... | 2.0–10.0 R⊙ | 4.5 R⊙ |
| Twind (near surface) | ... | ... | 1400–2400 K | 1600 K |
| Opening angle | ... | ... | 25–55° | 45° |
| Ṁ | ... | ... | 10−6–10−12 M⊙yr−1 | 10−7 M⊙yr−1 |
Notes. Computed using the TORUS radiative transfer model (Harries 2000) for the BK12 model scenario. qdist is the power law of the grain size distribution. The best fit values are those of the BK12 prescription rather than the IN05 or THM07 models. αdisk is fixed at (βdisk + 1). References.(1) Akeson et al. (2005); (2) Unruh et al. (2004); (3) Jeffers et al. (2014).
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