Open Access
Table 1
Parameters describing the four simulated stellar models.
| Spectral type | K8V | K2V | G2V | F5V |
|---|---|---|---|---|
| Teff (K) | 4005 | 5000 | 5766 | 6506 |
| log (g) | 4.66 | 4.59 | 4.44 | 4.24 |
| Hp(z = 0)(km) | 60 | 100 | 182 | 348 |
| Lx, Ly (km) | 2200 | 3500 | 6000 | 15000 |
| Lz (km) | 968 | 1540 | 3072 | 7800 |
| Below z = 0 (km) | 748 | 1190 | 2412 | 6150 |
| Above z = 0 (km) | 220 | 350 | 660 | 1650 |
| Δx, Δy, Δz (km) | 2.93 | 4.67 | 8.00 | 20.00 |
| Lgran (km) | 354 | 609 | 990 | 2490 |
| Nkin | 27 | 20 | 18 | 20 |
| Nsat | 20 | 32 | 36 | 34 |
Notes. See text in Sect. 2.1 for more details. Teff, Lgran, and HP were evaluated as time averages during the kinematic phase of the simulations. For more details, the reader can refer to Riva et al. (2024).
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