Table 2.
Planetary system parameters used as input for simulations.
| Star |
Companion |
|||||||||
|---|---|---|---|---|---|---|---|---|---|---|
| System | H | Ks | Teff(a) | log g(a) | Sep. | ΔH | ΔK | Teff(a) | log g(a) | References |
| [K] | [dex] | [mas] | [mag] | [mag] | [K] | [dex] | ||||
| β Pic | 3.54 | 3.53 | 8052 [8100] | 4.15 [4.0] | 300 | 10.0 | 9.2 | 1650 [1700] | < 4.7 [4.0] | 1, 2, 3 |
| HIP 65426 | 6.85 | 6.77 | 8840 [8800] | 4.23 [4.0] | 830 | 11.1 | 10.0 | 1450 [1500] | < 4.5 [4.0] | 4, 5 |
| 51 Eri | 4.77 | 4.54 | 7256 [7200] | 4.13 [4.0] | 452 | 14.8 | 12.9 | 760 [700] | 4.3 [4.0] | 6, 7, 8 |
| PDS 70 | 8.82 | 8.54 | 3972 [4000] | 3.90 [4.0] | 199 | 9.12 | 7.8 | 1200 [1200] | 3.9 [4.0] | 9, 10 |
Notes.
The Teff and log g values from the literature are reported on the left side of the columns, while the values used for the models in the simulation are reported between brackets on the right side of the columns.
References. (1) Bonnefoy et al. (2013); (2) Lagrange et al. (2019); (3) Chilcote et al. (2017); (4) Chauvin et al. (2017a); (5) Cheetham et al. (2019); (6) Macintosh et al. (2015); (7) Samland et al. (2017); (8) Rajan et al. (2017); (9) Keppler et al. (2018); (10) Müller et al. (2018).
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