Table 3
Observational disk properties of different pressure bump models.
| Name (1) | rgap (au) (2) | Amax (3) | Tfin (Myr) (4) |  (M⊕) (5) |
 (M⊕) (6) |
 (M⊕) (7) |
Md,obs (M⊕) (8) | F1,3mm (mJy) (9) | F3.0mm (mJy) (10) | αmm (11) | Rd,68% (au) (12) | Rd,90% (au) (13) |  (14) |
 (15) |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Inner Bump | 10 | 2 | 0.10 | 115 | 100 | 102 | 9.9 | 17.9 | 2.0 | 2.6 | 13 | 16 | 35 | 0.41 |
| Fiducial | 30 | 2 | 0.10 | 87.3 | 77.7 | 71.2 | 26.9 | 48.5 | 5.1 | 2.7 | 38 | 42 | 3.5 | 0.70 |
| Smaller A | 30 | 1 | 0.10 | 16.5 | 2.4 | 11.4 | 11.8 | 21.3 | 1.2 | 3.4 | 36 | 41 | 0.26 | 0.19 |
| Bigger A | 30 | 4 | 0.10 | 94.7 | 92.4 | 77.2 | 24.7 | 44.6 | 4.8 | 2.7 | 40 | 44 | 3.8 | 0.66 |
| Strong A | 30 | 10 | 0.10 | 97.0 | 96.3 | 78.7 | 23.1 | 41.7 | 4.6 | 2.6 | 42 | 46 | 3.9 | 0.59 |
| Fast T | 30 | 2 | 0.05 | 90.5 | 80.8 | 74.1 | 27.2 | 49.1 | 5.2 | 2.7 | 38 | 42 | 3.6 | 0.71 |
| Long T | 30 | 2 | 0.50 | 52.5 | 44.9 | 41.6 | 24.0 | 43.2 | 3.9 | 2.9 | 38 | 42 | 1.8 | 0.63 |
| Longer T | 30 | 2 | 1.0 | 30.6 | 24.9 | 23.0 | 19.4 | 35.0 | 2.4 | 3.2 | 38 | 42 | 0.86 | 0.47 |
| Outer Bump | 80 | 3 | 0.20 | 38.9 | 37.0 | 24.2 | 19.0 | 34.3 | 1.6 | 3.7 | 106 | 110 | 0.27 | 0.24 |
| Two Bumps | 30&80 | 2&3 | 0.1&0.2 | 88.1 | 79.6 | 66.3 | 32.7 | 58.9 | 4.8 | 3.0 | 39 | 100 | 1.9 | 0.60 |
| No Bump | – | – | – | 6.8 | 1.7 | 3.4 | 6.5 | 11.7 | 0.5 | 3.7 | 35 | 55 | 0.02 | 0.02 |
Notes. (1) Given name of the pressure bump model. (2-4) Various model parameters as described in Sect. 2.2. (5, 6) Total dust masses at 1 Myr and 3 Myr of disk evolution. (7) Dust mass of grains larger than 0.1 mm at 1 Myr. (8) Observed disk dust mass (Eq. (20)). (9, 10) Synthetic fluxes of the disk at 1.3 mm and 3.0 mm. (11) Millimetre spectral index (Eq. (19)). (12, 13) Dust disk radii that encloses either 68% or 90% of the 1.3 mm flux. (14, 15) Peak absorption and observed optical depth at location of dust ring, both at λ = 1.3 mm (Eqs. (21), (22)).
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