Table 2
Disk parameters utilized in constructing the simulation.
| Gaseous disk | Dusty disk | ||||
|---|---|---|---|---|---|
| Name | Unit | Value | Name | Unit | Value |
| Σ0 | g cm−2 | 102 | Σ0,dust | g cm−2 | 1.0 |
| T0 | K | 127.9 | ρs | g cm−3 | 3.0 |
| rmin | au | 1.25 | s1 | mm | 0.2 |
| rmax | au | 12.5 | s2 | mm | 1.0 |
| r0 | au | 5.0 | s3 | mm | 4.6 |
| p1 | − | 1.0 | St1 | 10−2 | 0.2 |
| p2 | − | 0.5 | St2 | 10−2 | 1.1 |
| St3 | 10−2 | 5.1 | |||
Notes. Gaseous disk: we initialised the gas disk with a surface density Σ0 and temperature T0 at the reference radius r0 by following power laws with exponents p1 and p2, respectively (see Equations (6) and (7)). The disk extends from rmin to rmax. Dusty disk: the dust disk is initialized equal to the gaseous disk but with a different surface density Σ0,dust at r0. The dust disk is composed of three dust grains: s1, s2, and s3 with the corresponding Stokes number St1, St2, and St3, respectively, having all of them an intrinsic grain density of ρs.
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