Table 1
Initial set-up hierarchical triple models.
| Parameter | Unit | Initial value |
|---|---|---|
| M1 | (M⊙) | 1.6 |
| M2 | (M⊙) | 0.4 |
| R1,accr | (R⊙) | 258 |
| R2,accr | (R⊙) | 8.6 |
| Ṁ | (M⊙ yr−1) | 1.1 × 10−6 |
| T1 | (K) | 2800 |
| ai | (au) | 5 |
| ao | (au) | 35 |
| Rbound | (au) | 1500 |
| tmax | (Po) | 4 |
Notes. The set-up parameters are the same for all hierarchical triple models: M1, M2, R1,accr, and R2,accr are the initial masses and accretion radii of the primary (AGB) and secondary (companion) star of the inner binary, M is the mass-loss rate of the AGB star, and T1 its effective temperature, ai and ao are the semi-major axes of the inner and outer binary, and Rbound is the boundary radius beyond which gas particles are killed. The simulations are computed over at least four outer orbital periods (Po).
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.