Table 1
Parameter setup of each simulation A through U.
| Simulation | Binary system | h | α | Σ0 (M⊙/au2) | Self-gravity | Boundary | α Σ |
|
|
|||||||
| A | Kepler-16 | 0.03 | 10-3 | 1.0 × 10-4 | No | Rigid | 1.5 |
| B | Kepler-16 | 0.05 | 10-3 | 1.0 × 10-4 | No | Rigid | 1.5 |
| C | Kepler-16 | 0.03 | 10-2 | 1.0 × 10-4 | No | Rigid | 1.5 |
| D | Kepler-16 | 0.05 | 10-2 | 1.0 × 10-4 | No | Rigid | 1.5 |
| E | Kepler-34 | 0.03 | 10-3 | 1.0 × 10-4 | No | Rigid | 1.5 |
| F | Kepler-34 | 0.05 | 10-3 | 1.0 × 10-4 | No | Rigid | 1.5 |
| G | Kepler-34 | 0.03 | 10-2 | 1.0 × 10-4 | No | Rigid | 1.5 |
| H | Kepler-34 | 0.05 | 10-2 | 1.0 × 10-4 | No | Rigid | 1.5 |
|
|
|||||||
| I | Kepler-16 | 0.03 | 10-3 | 1.0 × 10-4 | Yes | Rigid | 1.5 |
| J | Kepler-16 | 0.05 | 10-3 | 1.0 × 10-4 | Yes | Rigid | 1.5 |
| K | Kepler-34 | 0.03 | 10-3 | 1.0 × 10-4 | Yes | Rigid | 1.5 |
| L | Kepler-34 | 0.05 | 10-3 | 1.0 × 10-4 | Yes | Rigid | 1.5 |
|
|
|||||||
| M | Kepler-16 | 0.05 | 10-3 | 1.0 × 10-4 | No | Open | 1.5 |
| N | Kepler-34 | 0.05 | 10-3 | 1.0 × 10-4 | No | Open | 1.5 |
|
|
|||||||
| O | Kepler-16 | 0.05 | 10-3 | 5.0 × 10-4 | Yes | Rigid | 1.5 |
| P | Kepler-16 | 0.05 | 10-3 | 1.0 × 10-3 | Yes | Rigid | 1.5 |
| Q | Kepler-16 | 0.05 | 10-3 | 2.5 × 10-3 | Yes | Rigid | 1.5 |
| R | Kepler-16 | 0.05 | 10-3 | 5.0 × 10-4 | No | Rigid | 1.5 |
| S | Kepler-16 | 0.05 | 10-3 | 1.0 × 10-3 | No | Rigid | 1.5 |
| T | Kepler-16 | 0.05 | 10-3 | 2.5 × 10-3 | No | Rigid | 1.5 |
|
|
|||||||
| U | Kepler-16 | 0.05 | 10-3 | 1.0 × 10-4 | Yes | Rigid | 0.5 |
Notes. A–H test the effect of varying aspect ratio, alpha-viscosity and central binary type on non self-gravitating disks. I–L test the inclusion of self-gravity at standard surface density. M–N investigate the inclusion of an open boundary. O–T look at the relevance of self-gravity in more detail by increasing the surface density of the disk. U tests the dependency of the disk evolution on the surface density profile exponent, αΣ.
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