Table 3
Eccentricity and semi-major axis of the cavity edge (ecav, acav), peak density (epeak, apeak), and planetary orbit (epl, apl).
| h/r = 0.03 | h/r = 0.05 | |||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| No planet | With planet | No planet | With planet | |||||||||
| Setup | 0.15 | 0.25 | 0.35 | 0.15 | 0.25 | 0.35 | 0.15 | 0.25 | 0.35 | 0.15 | 0.25 | 0.35 |
| ecav | 0.089 | 0.093 | 0.122 | 0.015 | 0.032 | 0.027 | 0.153 | 0.196 | 0.206 | 0.028 | 0.043 | 0.044 |
| acav | 3.87 | 4.25 | 4.59 | 3.79 | 4.09 | 4.47 | 3.76 | 4.13 | 4.52 | 3.72 | 3.90 | 3.99 |
| epeak | 0.061 | 0.069 | 0.094 | 0.049 | 0.046 | 0.034 | 0.028 | 0.056 | 0.079 | 0.049 | 0.045 | 0.037 |
| apeak | 4.55 | 4.91 | 5.24 | 5.39 | 5.78 | 6.39 | 5.79 | 6.05 | 6.22 | 6.06 | 6.27 | 6.57 |
| qpeak | 1.43 | 1.44 | 1.60 | 1.16 | 1.16 | 1.10 | 1.40 | 1.60 | 1.76 | 1.11 | 1.18 | 1.17 |
| epl | 0.019 | 0.020 | 0.024 | 0.016 | 0.017 | 0.020 | ||||||
| apl | 3.34 | 3.55 | 3.74 | 3.58 | 3.83 | 3.99 | ||||||
Notes. Values were calculated by taking the median of the last 1000 binary orbits. The ratio between the brightest and dimmest part of the ring peak is shown as qpeak. The highlighted epeak and qpeak are the values consistent with the observations, as described in Sect. 5.2.
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