Table 3
Overview of parameter ranges used in the modeling.
| Parameter | Unit | Range | Best fit | Uncertainties |
|---|---|---|---|---|
| Disk | ||||
| rin | au | 0.1−100.0 | 16.0 |  |
| rout | au | 100.0−300.0 | 172.0 |  |
| hout∕rout | 0.05−0.50 | 0.22 |  |
|
| p | 0.5−2.0 | 0.87 |  |
|
| k | 1.0−5.0 | 1.185 |  |
|
| Σout | g cm−2 | (0.1−10) × 10−2 | 4.6 × 10−2 |  |
| ϕ | deg | 60.0−90.0 | 88.0 |  |
| PA | deg | −20.0 to −40.0 | − 32.0 |  |
| Envelope | ||||
| Rin | au | 0.1 | 0.1 | Fixed |
| Rout | au | 900 | 900 | Fixed |
| ρout | g cm−3 | (0.1−90) × 10−20 | 6.1 × 10−20 |  |
| γ | − 0.01 to −0.5 | − 0.10 |  |
|
| P.C. | deg | 40.0 | 40.0 | Fixed |
| Star | ||||
| r⋆ | R⊙ | 2.0 | 2.0 | Fixed |
| M⋆ | M⊙ | 0.55 | 0.55 | Fixed |
| T⋆ | K | 3000−5000 | 4000 |  |
| AV | mag | 1.0−30.0 | 13.06 |  |
| Distance | pc | 140.0 | 140.0 | Fixed |
| Grain size distribution | ||||
 |
μm | 0.25−100 000 | 50 000 |  |
 |
μm | 0.25−100 00 | 110 |  |
 |
μm | 0.01 | 0.01 | Fixed |
 |
μm | 0.01 | 0.01 | Fixed |
Notes. rin : inner radius of the disk. rout : outer radius of the disk. hout ∕rout: ratio of the pressure scale height to the radius at rout. p: power exponent of the radial surface density distribution. k: flare index. Σout : surface density of the disk at the outer radius. ϕ: inclination angle of the disk. Rin: inner radius of the envelope. Rout: outer radius of the envelope. ρout: density of the envelope at the outer radius. γ: radial density distribution power exponent. P.C.: radius of the polar cavity in the envelope. r⋆ : radius of the star. M⋆ : mass of the star, fitted with a Keplerian disk in the 12CO J = 2− 1 velocity field (Launhardt et al., in prep.). T⋆: effective surface temperature of the star. PA: rotation of the major axis in the image plane. AV : visual extinction. Distance: distance to the Sun. 
: maximum dust grain size in the disk. 
: maximum dust grain size in the envelope. 
: minimum dust grain size in the disk. 
: minimum dust grain size in the envelope. Uncertainties: defined by 
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