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Table 10

Stellar parameters obtained from the optical analysis using the Linear10−025 clumping law.

Star Teff [kK] log g [dex] log Q YHe υmic [km s−1] β
HD 46223 43.4 ± 0.9 3.83 ± 0.07 −13.1 ± 0.1 0.10 ± 0.03 10.2 ± 5.2 >1.0
HD 15629 42.3 ± 1.8 3.78 ± 0.10 −13.1 ± 0.1 0.12 ± 0.03 12.4 ± 7.4 >1.0
HD 46150 40.0 ± 0.8 3.80 ± 0.08 −13.4 ± 0.2 0.10 ± 0.03 <11.8 >0.8
H D217086 37.0 ± 1.0 3.60 ± 0.10 −13.5 ± 1.1 0.11 ± 0.03 12.4 ± 7.4 1.0 ± 0.2
HD 149757 32.5 ± 0.9 3.82 ± 0.17 −14.0 ± 1.0 0.11 ± 0.03 12.0 ± 7.0 >0.8
HD 190864 37.2 ± 0.8 3.60 ± 0.10 −13.1 ± 0.1 0.12 ± 0.03 10.4 ± 5.4 >0.8
HD 203064 35.0 ± 0.5 3.50 ± 0.06 −13.1 ± 0.1 0.10 ± 0.03 >13.7 1.0 ± 0.2
HD 15570 39.8 ± 0.6 3.48 ± 0.07 −12.4 ± 0.1 0.10 ± 0.03 <19.9 1.1 ± 0.1
HD 14947 38.0 ± 0.2 3.50 ± 0.03 −12.5 ± 0.1 0.14 ± 0.03 <11.3 >1.2
HD 30614 29.1 ± 0.2 <2.83 −12.6 ± 0.1 >0.20 >18.4 1.1 ± 0.1
HD 210809 31.0 ± 0.8 3.05 ± 0.12 −12.7 ± 0.1 >0.13 >14.9 1.1 ± 0.2
HD 209975 31.5 ± 0.6 3.26 ± 0.09 −13.1 ± 0.2 0.10 ± 0.03 <12.1 1.0 ± 0.2

Notes. Upper and lower limits refer to the corresponding parameter ranges of our model grids only (see Table 9).

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