Table 2
Initial conditions that were used for the 2D FARGO simulations described in Sect. 2.3.
| FARGO parameter | value |
|---|---|
| Sigma0 (g cm‒2) | 10, 100 |
| SigmaSlope | 1. |
| SigmaFloor (Σ0) | 10−9 |
| AlphaViscosity | 6.9 × 10−4 |
| AspectRatio | 0.1 |
| FlaringIndex | 0.25 |
| l0 (au) | 5. |
| m0 (M⊙) | 0.7 |
| mu | 2.35 |
| Nrad | 256 |
| Nsec | 388 |
| Rmin (l0) | 0.08 |
| Rmax (l0) | 5. |
| RadialSpacing | Logarithmic |
| InnerBoundary | Viscous |
| OuterBoundary | Viscous |
| Adiabatic | No |
| PlanetMass (MJ) | 1. |
| PlanetDistance (au) | 5. |
Notes. The parameters are given in the name convention employed in the FARGO executable files. If a parameter is not specified, the default value is used. We note that FARGO employs code units, which are set by the base mass
m0, the base length
l0 and the time per orbit 
, where
G is the gravitational constant and Ω0
the Keplerian orbital frequency.
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