Table 1
Overview of the configuration of the twelve models (input values and orbital velocities).
| Model | vini | a | Mcomp | vAGB | vcomp |
|---|---|---|---|---|---|
| (km s−1) | (au) | (M⊙) | (km s−1) | (km s−1) | |
| S90FAST | 20.0 | 9.0 | 1.0 | 6.3 | 9.4 |
| S40FAST | 20.0 | 4.0 | 1.0 | 9.4 | 14.1 |
| S25FAST | 20.0 | 2.5 | 1.0 | 11.9 | 17.9 |
| P90FAST | 20.0 | 9.0 | 0.01 | 0.1 | 12.1 |
| P40FAST | 20.0 | 4.0 | 0.01 | 0.1 | 18.2 |
| P25FAST | 20.0 | 2.5 | 0.01 | 0.2 | 23.0 |
| S90SLOW | 5.0 | 9.0 | 1.0 | 6.3 | 9.4 |
| S40SLOW | 5.0 | 4.0 | 1.0 | 9.4 | 14.1 |
| S25SLOW | 5.0 | 2.5 | 1.0 | 11.9 | 17.9 |
| P90SLOW | 5.0 | 9.0 | 0.01 | 0.1 | 12.1 |
| P40SLOW | 5.0 | 4.0 | 0.01 | 0.1 | 18.2 |
| P25SLOW | 5.0 | 2.5 | 0.01 | 0.2 | 23.0 |
Notes. Here, vini is the initial velocity (input), a the binary separation (input) and Mcomp the input mass of the companion (0.01 M⊙≈ 10 MJup). The naming of the models is abbreviated according to ‘Mcomp + 10a + windtype’, where Mcomp is given by ‘S’ or ‘P’, standing for ‘stellar’ and ‘planetary’, respectively. ‘FAST’ refers to a wind initiated with vini = 20 km s−1 and Ṁ = 10−4 M⊙ yr−1, and ‘SLOW’ to a wind with vini = 5 km s−1 and Ṁ = 2 × 10−7 M⊙ yr−1. vAGB and vcomp are the orbital velocity of the AGB star and companion, respectively. Following applies for all models: MAGB = 1.5 M⊙, e = 0, γ = 1.2. More detailsabout the simulations can be found online: http://doi.org/10.5281/zenodo.5070188.
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