Table 2
Literature values for stars with results from detailed modelling.
| Star | Δν [ μHz] | Teff [K ] | [Fe/H] [dex ] | M / M ⊙ | R / R ⊙ | τ [Gyr ] | References |
|
|
|||||||
| Kepler-37 | 178.7 ± 1.4 * | 5417 ± 75 | −0.32 ± 0.07 | 0.802 ± 0.068 | 0.770 ± 0.026 | ~6 | 1 |
| α Cen B | 161.1 ± 0.1 * | 5260 ± 50 | 0.24 ± 0.05 | 0.934 ± 0.0061 | 0.863 ± 0.005 | 6.52 ± 0.30 | 2, 3, 4, 5, 6 |
| Kepler-10 | 118.2 ± 0.2 * | 5643 ± 75 | −0.15 ± 0.07 | 0.913 ± 0.022 | 1.065 ± 0.009 | 10.41 ± 1.36 | 7, 8, 9 |
| α Cen A | 105.5 ± 0.1 * | 5810 ± 50 | 0.22 ± 0.05 | 1.105 ± 0.0070 | 1.224 ± 0.003 | 6.52 ± 0.30 | 2, 3, 4, 5, 6 |
| Perky | 104 ± 0.5 * | 6000 ± 200 | −0.09 ± 0.1 | 1.11 ± 0.05 | 1.23 ± 0.02 | 4.87 ± 0.50 | 10 |
| Kepler-68 | 101.51 ± 0.09 * | 5793 ± 44 | 0.12 ± 0.04 | 1.079 ± 0.051 | 1.243 ± 0.019 | 6.3 ± 1.7 | 11 |
| Kepler-65 | 90.0 ± 0.5 * | 6211 ± 66 | 0.17 ± 0.06 | 1.25 ± 0.06 | 1.41 ± 0.03 | 2.9 ± 0.7 | 12 |
| μ Arae | 90 ± 1.1 | 5813 ± 40 | 0.32 ± 0.05 | 1.10 ± 0.02 | 1.36 ± 0.06 | 6.34 ± 0.80 | 13, 14 |
| Dushera | 88 ± 0.6 * | 6200 ± 200 | 0.0 ± 0.15 | 1.15 ± 0.04 | 1.39 ± 0.01 | 3.80 ± 0.37 | 10 |
| Kepler-50 | 76.0 ± 0.9 | 6225 ± 66 | 0.03 ± 0.06 | 1.24 ± 0.05 | 1.58 ± 0.02 | 3.8 ± 0.80 | 12 |
| Kepler-36 | 67.9 ± 1.2 | 5911 ± 66 | −0.20 ± 0.06 | 1.071 ± 0.043 | 1.626 ± 0.019 | 6.8 ± 1.0 | 15 |
| HAT-P-7 | 59.22 ± 0.59 * | 6350 ± 80 | 0.26 ± 0.08 | 1.53 ± 0.005 | 1.997 ± 0.003 | 1.81 ± 0.08 | 16, 17, 18 |
| β Hyi | 57.24 ± 0.16 * | 5840 ± 59 | −0.04 ± 0.10 | 1.085 ± 0.028 | 1.809 ± 0.015 | 6.40 ± 0.56 | 19, 20, 21, 22 |
| Kepler-7 | 56.4 ± 1.7 | 5933 ± 44 | 0.11 ± 0.03 | 1.359 ± 0.031 | 1.966 ± 0.013 | 3.3 ± 0.4 | 18, 23, 24 |
| Procyon | 56.0 * | 6494 ± 48 | 0.02 ± 0.10 | 1.461 ± 0.025 | 2.059 ± 0.015 | 1.87 ± 0.13 | 19, 25, 26 |
| η Boo | 39.9 ± 0.1 * | 6030 ± 80 | 0.24 ± 0.07 | 1.57 ± 0.07 | 2.701 ± 0.040 | 2.67 ± 0.10 | 19, 27 |
Notes.
Reference. (1) Barclay et al. (2013); (2) Eggenberger et al. (2004); (3) Pourbaix et al. (2002); (4) Kervella et al. (2003); (5) Bouchy & Carrier (2002); (6) Carrier & Bourban (2003); (7) Batalha et al. (2011); (8) Torres et al. (2012); (9) Fogtmann-Schulz et al. (2014); (10) Silva Aguirre et al. (2013); (11) Gilliland et al. (2013); (12) Chaplin et al. (2013); (13) Soriano & Vauclair (2010); (14) Santos et al. (2004); (15) Carter et al. (2012); (16) Pál et al. (2008); (17) Lund et al. (in prep.); (18) Huber et al. (2013); (19) Bruntt et al. (2010); (20) Bedding et al. (2007); (21) Kjeldsen et al. (2008); (22) Brandão et al. (2011); (23) Latham et al. (2010); (24) Demory et al. (2011); (25) Bedding et al. (2010); (26) Liebert et al. (2013); (27) Carrier et al. (2005).
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