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Table 3

Parameters of the preferred models for the full sample of sources.

Source M L i d Rc infall θcav ncav Exf Mdisk 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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