Table 1
Characteristic parameters for the models.
| Model |  (M⊙) |
 (M⊙) |
 (M⊕) |
Mpeb (M⊕) |  (AU) |
 (AU) |
|---|---|---|---|---|---|---|
| α = 10−2 | 0.37 | 0.115 | 260.78 | – | 287.10 | 1159.9 |
| α = 10−3 | 0.32 | 0.172 | 106.47 | 14.24 | 118.87 | 224.73 |
| α = 10−4 | 0.27 | 0.225 | 983.22 | 884.60 | 9.30 | 213.99 |
| α = 10−4, ufrag = 0.5 m s−1 | 0.30 | 0.192 | 744.26 | 32.17 | 110.45 | 189.32 |
| α = 10−4, ufrag = 1.0 m s−1 | 0.31 | 0.187 | 731.49 | 263.64 | 82.32 | 198.82 |
| α = 10−3, ζ = 0.01 | 0.32 | 0.172 | 573.03 | 75.96 | 118.87 | 224.73 |
| α = 10−4, ζ = 0.01 | 0.27 | 0.225 | 750.75 | 184.14 | 9.30 | 213.99 |
| δ = 10−3 + αGI | 0.32 | 0.176 | 492.65 | 23.67 | 116.00 | 230.30 |
| δ = 10−4 + αGI | 0.29 | 0.205 | 849.85 | 142.57 | 110.45 | 180.27 |
Notes. 
is the final mass of the central star, 
and 
are the gas and dust disk radii containing 98% of total gas and dust mass, respectively, 
and 
are the corresponding gas and dust masses. All the values are shown at the end of simulations. Mpeb is the total mass of pebbles averaged over the final 100 kyr of simulations.
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