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Table 3
Parameters of the preferred models for the full sample of sources.
Source | M⋆ | L⋆ | i | d | ![]() |
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Rc | Ṁinfall | θcav | ncav | Exf | Mdisk | ![]() |
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Dust fraction | D1 SH | D2 SH | ![]() |
|
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
PA | (M⊙) | (L⊙) | (°) | (kpc) | (au) | (au) | (au) | (M⊙ yr−1) | (°) | (g cm−3) | (M⊙) | (au) | (au) | (°) | |||||
W33A | 25 | 49 270 | 120 | 2.4 | 18 (Rsub) | 5 × 105 | 500 | 7.4 × 10−4 | 20 | 1 × 10−19 | 0 | 1 | 18 (Rsub) | 500 | 0.2 | 0.11 | 0.22 | 0 | 30 |
G305.20+0.21 | 25 | 48 500 | 35 | 4 | 60 | 5 × 105 | 2000 | 7.5 × 10−4 | 12 | 8 × 10−21 | 0 | 1 | 60 | 2000 | 1 | 0.1 | – | 1 | 55 |
NGC 2264 IRS1 | 8 | 4200 | 15 | 0.74 | 4 (Rsub) | 5 × 105 | 500 | 9 × 10−4 | 25 | 8 × 10−21 | 0.25 | 0.3 | 4 (Rsub) | 500 | 0.2 | 0.4 | 0.8 | 25 | −18.5 |
S255 IRS3 | 20 | 21 550 | 120 | 1.8 | 12 (Rsub) | 1 × 105 | 500 | 7.5 × 10−8 | 20 | 6 × 10−19 | 0 | 1 | 12 (Rsub) | 500 | 0.2 | 0.1 | 0.1 | 70 | 67 |
IRAS 17216-3801 | 38 | 172 000 | 15 | 3.08 | 1 | 5 × 105 | 1000 | 4 × 10−3 | 40 | 9 × 10−21 | 1 | 1 | 100 | 1000 | 0.2 | 0.4 | 0.7 | 60 | 320 |
Mon R2 IRS2 | 15 | 5500 | 130 | 0.84 | 20 | 5 × 105 | 2000 | 9.5 × 10−4 | 30 | 3 × 10−21 | 0 | 0.1 | 20 | 2000 | 0.2 | 0.4 | 0.8 | 25 | 190 |
M8EIR | 13.5 | 12 100 | 25 | 1.33 | 30 | 5 × 105 | 2000 | 1 × 10−3 | 25 | 8 × 10−21 | 0.25 | 0.1 | 30 | 2000 | 0.2 | 0.4 | 0.8 | 25 | 260 |
AFGL 2136 | 20 | 151 000 | 60 | 2.2 | 125 | 1 × 105 | 2000 | 3 × 10−4 | 22.5 | 3 × 10−19 | 0 | 20 | 125 | 2000 | 0.2 | 0.375 | 0.375 | 60 | −35 |
Notes. PA is shorthand for position angle and is defined as east from north. Exf. stands for cavity density exponent (Whitney et al. 2013), D1 SH is short for ‘disk 1 scale-height’ and D2 SH is short for ‘disk 2 scale-height’.
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