Table 2
Warped disk model parameters, most of which have been unchanged from the best fit model in Tobin et al. (2013).
| Parameters | Description | Values |
|---|---|---|
| γ’s | Number of photons | 1 × 108 |
| R⋆(R⊙) | Stellar radius | 2.09 |
| T⋆(K) | Stellar temperature | 4000 |
| M⋆(M⊙) | Stellar mass | 0.5 |
| Mdisk(M⊙) | Disk mass | 0.005 |
| h (100 AU) | Disk scale height at 100 AU | 48.0 |
| H0 (R⋆) | Disk scale height at R⋆ | 0.03 |
| α | Disk radial density exponent | 2.5 |
| β | Disk scale height exponent | 1.3 |
| Ṁdisk (M⊙ yr−1) | Disk accretion rate | 1.5 × 10−6 |
| Rtrunc (R⋆) | Magnetosphere co-rotation radius | 3.0 |
| Fspot | Fractional area of accretion hotspot | 0.01 |
| Rdisk, min (R⋆, AU) | Disk inner radius | 14.25, 0.14 |
| Rdisk, max (AU) | Disk outer radius | 125 |
| Renv, min (R⋆) | Envelope inner radius | 42.75 |
| Renv, max (AU) | Envelope outer radius | 15000 |
| Ṁenv (M⊙ yr−1) | Envelope mass infall rate | 4.5 × 10−6 |
| ρ1 AU (g cm−3) | Envelope density at 1 AU | 7.25 × 10−14 |
| bout | Outer cavity shape exponent | 1.5 |
| θopen, out (°) | Outer cavity opening angle | 20 |
| ρc (g cm−3) | Cavity density | 0 |
| βdust, mm | Millimeter dust spectral index | 0.25 |
| Warp height | Multiplicative factor of warp scale height above disk scale height | 10.0 |
| n | Exponent for azimuthal disk warp (cosn) | 41 |
| θ (°) | Inclination angles of high S/N images | 85.0 |
| ϕ (°) | Azimuthal angles | 0,15.0,30.0,…,180.0 |
| λ (μm) | wavelength | 2.15 |
Notes. Parameters most relevant to this result are in boldface and parameters that have been adjusted from the value in the best fit model are italicized. The stellar mass is only used in setting the density structure, changing this to the measured protostar mass would require increasing the envelope infall rate to maintain the same density structure.
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