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Table 6

Stellar parameters obtained from the NIR analysis using unclumped models.

Star Teff [kK] log g [dex] log Q YHe υmic [km s−1] β
HD 46223 41.2 ± 1.4 3.79 ± 0.10 −12.7 ± 0.2 <0.10 >5.0 >0.9
HD 15629 39.5 ± 1.7 3.66 ± 0.17 −13.2 ± 0.7 <0.09 12.4 ± 7.4 >0.8
HD 46150 39.6 ± 1.0 3.85 ± 0.12 −12.9 ± 0.3 <0.08 <18.5 >0.8
HD 217086 36.9 ± 1.1 3.86 ± 0.15 −13.8 ± 1.2 0.15 ± 0.07 >5.0 >0.8
HD 149757 32.3 ± 1.7 3.58 ± 0.31 −13.7 ± 1.3 0.19 ± 0.10 >5.0 >0.8
HD 190864 36.8 ± 1.0 3.64± 0.14 −12.7 ± 0.3 0.21 ± 0.09 12.4 ± 7.4 >0.9
HD 203064 34.3 ± 1.5 3.70 ± 0.32 −12.5 ± 0.2 0.20 ± 0.10 >5.0 >1.0
HD 15570 38.8 ± 1.8 3.55 ± 0.15 −11.9 ± 0.1 0.10 ± 0.03 <19.9 <1.0
HD 14947 43.6 ± 2.8 4.03 ± 0.36 −12.5 ± 0.5 >0.17 12.4 ± 7.4 >0.9
HD 30614 27.6 ± 0.8 2.78 ± 0.08 −12.0 ± 0.1 <0.17 >5.0 <1.2
HD 210809 35.4 ± 1.2 >3.80 −12.8 ± 0.3 >0.23 >10.4 >0.8
HD 209975 32.1 ± 1.3 3.33 ± 0.18 <−13.4 >0.12 15.9 ± 3.9 <1.2

Notes. Gravities do not include a centrifugal correction. For upper an lower limits see caption of Table 5.

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