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Table 1
Stellar parameters for each of the 15 stars studied here.
| Star | Mass | T eff | log g | [Fe/H] | B − V |
|
P rot a | |||
| [M⊙] | [K] | [cgs] | [days] | |||||||
|
|
||||||||||
| HD 224817 | 0.98 ± 0.06 | 5894 ± 22 | 4.36 ± 0.02 | –0.53 ± 0.02 | 0.55 | –4.96 | 13.0/13.5 | |||
| HD 21132 | 1.05 ± 0.07 | 6243 ± 34 | 4.60 ± 0.05 | –0.37 ± 0.02 | 0.49 | –4.90 | 7.2/7.3 | |||
| HD 22879 | 0.88 ± 0.06 | 5884 ± 33 | 4.52 ± 0.03 | –0.81 ± 0.02 | 0.56 | –4.91 | 12.8/13.1 | |||
| HD 31128 | 0.79 ± 0.05 | 6096 ± 67 | 4.90 ± 0.05 | –1.39 ± 0.04 | 0.41 | –4.88 b | – | |||
| HD 41248 | 0.94 ± 0.06 | 5713 ± 21 | 4.49 ± 0.03 | –0.37 ± 0.01 | 0.61 | –4.89 | 18.2/18.4 | |||
| HD 56274 | 0.90 ± 0.06 | 5734 ± 22 | 4.51 ± 0.03 | –0.54 ± 0.02 | 0.57 | –4.85 | 13.3/13.3 | |||
| HD 79601 | 0.94 ± 0.06 | 5834 ± 25 | 4.37 ± 0.04 | –0.60 ± 0.02 | 0.53 | –4.95 | 11.0/11.4 | |||
| HD 87838 | 1.03 ± 0.07 | 6118 ± 33 | 4.47 ± 0.03 | –0.40 ± 0.02 | 0.52 | –4.92 | 9.7/9.9 | |||
| HD 88725 | 0.87 ± 0.06 | 5654 ± 17 | 4.49 ± 0.03 | –0.64 ± 0.01 | 0.60 | –4.90 | 17.3/17.6 | |||
| HD 111777 | 0.87 ± 0.06 | 5666 ± 19 | 4.46 ± 0.03 | –0.68 ± 0.01 | 0.61 | –4.91 | 18.7/19.1 | |||
| HD 114076 | 0.80 ± 0.06 | 5069 ± 52 | 4.32 ± 0.09 | –0.47 ± 0.04 | 0.82 | –4.98 | 41.4/43.4 | |||
| HD 119173 | 0.96 ± 0.06 | 5779 ± 44 | 4.26 ± 0.04 | –0.62 ± 0.03 | 0.56 | –4.87 | 12.7/12.8 | |||
| HD 119949 | 1.09 ± 0.07 | 6359 ± 36 | 4.47 ± 0.04 | –0.41 ± 0.02 | 0.45 | –4.96 | 5.0/5.2 | |||
| HD 126793 | 0.92 ± 0.06 | 5910 ± 31 | 4.46 ± 0.03 | –0.71 ± 0.02 | 0.52 | –4.92 | 9.8/10.0 | |||
| HD 175607 | 0.81 ± 0.05 | 5392 ± 17 | 4.51 ± 0.03 | –0.61 ± 0.01 | 0.70 | –4.92 | 28.9/29.7 | |||
Notes.
(a)
The two values are estimated from the measurements using the calibrations from Noyes et al. (1984b) and Mamajek & Hillenbrand (2008), respectively.
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