Table 1
Systems that show evidence of spin-orbit commensurability (cf. Lanza 2022, Table 1).
| System | M/M⊙ (M⊙) | R/R⊙ (R⊙) | Teff (K) | a (au) | a/R | e | mp (Mj) | λso (deg) | Prot (day) | Porb (day) | Prot:Porb (m:n) | References |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| CoRoT-2 | 0.97 | 0.902 | 5625 | 0.0281 | 6.70 | 0.0 | 3.30 | 0.0 | 4.552 | 1.743 | 8:3 | 1, 2 |
| CoRoT-4 | 1.16 | 1.17 | 6190 | 0.0902 | 17.36 | <0.14 | 0.703 | 9.202 | 9.202 | 1:1 | 1, 3 | |
| CoRoT-6 | 1.05 | 1.025 | 6090 | 0.0854 | 17.94 | <0.18 | 2.95 | 6.35 | 8.887 | 5:7 | 1, 4 | |
| Kepler-13A | 1.72 | 1.74 | 7650 | 0.0355 | 4.44 | 4.9–8.1 | 23 ± 4 | 1.046 | 1.764 | 3:5 | 5, 6, 7 | |
| Kepler-17 | 1.16 | 1.05 | 5780 | 0.0268 | 5.48 | < 0.02 | 2.47 | 15 ± 15 | 11.89 | 1.486 | 8:1 | 1, 8, 9 |
| Kepler-63 | 0.984 | 0.90 | 5575 | 0.080 | 19.1 | <0.45 | < 0.38 | −110±20 | 5.401 | 9.424 | 3:5 | 10 |
| HAT-P-11 | 0.81 | 0.75 | 4780 | 0.053 | 15.6 | 0.218 | 0.0736 | 90 ± 30 | 30.5 | 4.888 | 6:1 | 11, 12, 13, 14 |
| τ Boo | 1.39 | 1.42 | 6400 | 0.049 | 7.40 | <0.011 | 6.13 | 3.31 | 3.3124 | 1:1 | 15, 16, 17 | |
| WASP-107 | 0.69 | 0.66 | 4430 | 0.0558 | 18.16 | 0.0 | 0.12 | 40-140 | 17.1 | 5.721 | 3:1 | 18 |
| AU Mic | 0.50 | 0.75 | 3700 | 0.0678 | 19.2 | 0.181 | 0.036 | −3 ± 10 | 4.8367 | 8.463 | 4:7 | 19, 20, 21 |
References. 1: Bonomo et al. (2017); 2: Lanza et al. (2009a); 3: Lanza et al. (2009b); 4: Lanza et al. (2011a); 5: Szabό et al. (2014); 6: Shporer et al. (2014); 7: Esteves et al. (2015); 8: Désert et al. (2011); 9: Lanza et al. (2019); 10: Sanchis-Ojeda et al. (2013); 11: Bakos et al. (2010); 12: Sanchis-Ojeda & Winn (2011); 13: Béky et al. (2014); 14: Yee et al. (2018); 15: Walker et al. (2008); 16: Brogi et al. (2012); 17: Borsa et al. (2015); 18: Dai & Winn (2017); 19: Szabό et al. (2021); 20: Cale et al. (2021); 21: Zicher et al. (2022).
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