Table 1
Initial orbital parameters.
| Row | a1 (au) | e1 | a2 (au) | e2 | i2 (°) | ω2 (°) | Ω2 (°) |
|---|---|---|---|---|---|---|---|
| 1 | 1.333 | 0.566 | 22.812 | 0.310 | 66.702 | 147.045 | 244.081 |
| 2 | 1.778 | 0.475 | 17.374 | 0.676 | 64.417 | 110.960 | 231.042 |
| 3 | 1.778 | 0.475 | 9.017 | 0.458 | 65.22 | 274.070 | 130.580 |
| 4 | 0.977 | 0.739 | 7.127 | 0.513 | 132.016 | 218.093 | 288.414 |
| 5 | 1.487 | 0.691 | 19.102 | 0.700 | 51.499 | 36.313 | 124.091 |
Notes. The table lists: the semimajor axis a2, eccentricity e2, inclination i2, argument of pericenter ω2, and ascending node longitude Ω2 associated with the Type-F particles of Fig. 11. Moreover, the semimajor axis a1 and the eccentricity e1 of the inner Jupiter-mass planet of each system are also specified. The rows are numbered from 1 to 5 from top to bottom of Fig. 11. It is important to note that the Type-F particles corresponding to rows 2–5 show values associated with (a1 ∕a2) or/and ɛ parameter slightly greater than 0.1.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.