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Table 5

Stellar parameters of the sample objects.

ID# Object Teff kK log g (cgs) y ξ v sin i/km s−1 ζ Rv E (B − V) mag B.C. mag Mevol M⊙ R R⊙ log L/L⊙ log τevol yr dspec pc dGaia (a) pc
1 HD 7902 14.1 2.13 0.089 9 36 35 3.16 0.58 −0.999 19.2 64 5.16 6.98 2900 2487
± 0.2 0.05 0.006 2 5 5 0.1 0.03 0.8 7 0.09 0.03 280
2 HD 14818 18.6 2.45 0.095 14 48 40 3.09 0.56 −1.645 23.6 49 5.41 6.89 2150 2121
± 0.3 0.07 0.008 2 6 5 0.1 0.03 1.9 6 0.11 0.03 250
3 HD 25914 13.6 1.81 0.092 11 35 40 2.97 0.76 −0.943 25.7 106 5.54 6.86 6030 5431
± 0.2 0.06 0.004 2 5 5 0.1 0.03 1.6 13 0.10 0.03 640
4 HD 36371 14.6 2.11 0.086 11 36 35 3.35 0.52 −1.081 21.1 68 5.28 6.94 1200 1214
± 0.3 0.06 0.005 2 5 5 0.1 0.03 1.2 8 0.10 0.03 130
5 HD 183143 12.8 1.76 0.099 7 37 27 3.3 1.22 −0.793 24.2 109 5.46 6.88 1530 2168
± 0.2 0.05 0.005 2 5 5 0.1 0.03 1.4 15 0.11 0.03 170
6 HD 184943 11.9 1.88 0.099 9 35 25 2.97 0.84 −0.600 17.7 82 5.07 7.02 4040 4090
± 0.2 0.05 0.002 2 6 5 0.1 0.03 0.8 10 0.10 0.04 400
7 HD 191243 14.0 2.64 0.087 8 27 25 2.88 0.33 −0.972 11.0 27 4.39 7.32 1220 1205
± 0.3 0.06 0.011 2 6 5 0.1 0.03 0.5 3 0.09 0.05 120
8 HD 199478 12.7 1.76 0.107 8 40 40 3.03 0.62 −0.783 24.0 111 5.46 6.88 2440 2423
± 0.2 0.05 0.004 2 6 5 0.1 0.03 1.3 12 0.09 0.03 230
9 HD 51309 15.6 2.59 0.081 10 30 35 3.08 0.11 −1.236 13.7 32 4.72 7.17 950 1108
± 0.4 0.05 0.003 2 6 5 0.1 0.03 0.5 4 0.09 0.04 90
10 HD 111990 17.2 2.62 0.089 12 40 40 3.3 0.45 −1.464 16.1 33 4.94 7.07 1940 2418
± 0.3 0.05 0.003 2 6 5 0.1 0.03 0.7 4 0.09 0.04 180
11 HD 119646 19.7 2.9 0.100 14 37 40 3.53 0.34 −1.781 15.4 23 4.87 7.10 1620 1721
± 0.2 0.07 0.009 2 6 5 0.1 0.03 1.2 3 0.11 0.05 190
12 HD 125288 13.7 2.77 0.094 6 23 30 3.65 0.30 0.934 9.3 21 4.14 7.46 390 438
± 0.3 0.05 0.007 2 4 5 0.1 0.03 0.3 2 0.09 0.05 40
13 HD 159110 19.5 3.42 0.095 3 17 15 3.3 0.22 −1.826 9.3 10 4.11 7.45 1290 1362
± 0.3 0.05 0.001 2 4 5 0.1 0.03 0.3 1 0.09 0.05 120
14 HD 164353 14.7 2.57 0.091 8 20 32 3.61 0.19 −1.081 12.6 31 4.60 7.22 620 797
± 0.3 0.05 0.004 2 4 5 0.1 0.03 0.4 4 0.09 0.04 60

Notes. Uncertainties are 1σ-values, except where noted otherwise. (a)Gaia Collaboration (2016, 2021) – distances and uncertainties correspond to ‘photogeometric distances’ and associated 14th and 86th confidence percentiles (Bailer-Jones et al. 2021).

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