Table C.1
Best-fit parameters obtained from fitting a power-law disk to the continuum visibilities after subtracting the envelope’s contribution.
| NOEMA: 203 GHz | ALMA Band 8: 390 GHz | |||||
|---|---|---|---|---|---|---|
| Parameter | TMC1A | L1527 | Elias29(a) | GSS30IRS1(b) | GSS30IRS3(c) | |
| q = 0.35 | ||||||
| p | 1.2 ± 0.2 | 0.6 ± 0.2 | 0.8 ± 0.2 | 1 ± 1 | 0.7 ± 0.2 | |
| Σ50 au | 1.0 ± 0.3 | 2.7 ± 0.4 | 0.3 ± 0.2 | 0.1 ± 0.4 | 1 ± 0.3 | g/cm−2 |
| Mdisk | 7 ± 3 | 23 ± 5 | 2.3 ± 1.6 | 0.7 ± 3 | 10 ± 3 | 10−3 × M⊙ |
| M>100 K | 2 | 3 | 0.4 | 0.2 | 2 | 10−3 × M⊙ |
| q = 0.40 | ||||||
| p | 1.2 ± 0.2 | 0.6 ± 0.2 | 0.8 ± 0.2 | 1 ± 1 | 0.7 ± 0.2 | |
| Σ50 au | 1.5 ± 0.4 | 3.9 ± 0.6 | 0.3 ± 0.2 | 0.2 ± 0.05 | 2 ± 0.5 | g cm−2 |
| Mdisk | 10 ± 4 | 34 ± 7 | 2.3 ± 1.6 | 1 ± 4 | 14 ± 4 | 10−3 × M⊙ |
| M>100 K | 5 | 12 | 1 | 0.7 | 2 | 10−3 × M⊙ |
| q = 0.5 | ||||||
| p | 1.3 ± 0.2 | 0.5 ± 0.2 | 0.9 ± 0.3 | 1 ± 1 | 0.6 ± 0.2 | |
| Σ50 au | 3.1 ± 0.8 | 11 ± 2 | 0.3 ± 0.2 | 0.3 ± 0.1 | 3 ± 1 | g cm−2 |
| Mdisk | 20 ± 9 | 100 ± 20 | 2.2 ± 1.6 | 2 ± 7 | 30 ± 7 | 10−3 × M⊙ |
| M>100 K | 7 | 12 | 0.5 | 0.5 | 4 | 10−3 × M⊙ |
Notes. The tabulated mass refers to the total mass of the disk using a gas-to-dust ratio of 100. (a) Only u − v distances between 200 and 730 kλ were fitted. (b)Only u − v distances between 200 and 800 kλ were fitted. Source located at edge of the primary beam. (c)Only u − v distances > 200 kλ were fitted.
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