Open Access
Table 11
As Table 10, but for the NIR analysis using the Linear10−025 clumping law.
Star | Teff [kK] | log g [dex] | log Q | YHe | υmic [km s−1] | β |
---|---|---|---|---|---|---|
HD 46223 | 42.7 ± 1.7 | 3.83 ± 0.10 | −14.1 ± 1.4 | <0.10 | >5.0 | <1.3 |
HD 15629 | 40.8 ± 1.2 | 3.85 ± 0.10 | −13.0 ± 1.3 | 0.10 ± 0.03 | <19.9 | >0.8 |
HD 46150 | 39.5 ± 0.8 | 3.85 ± 0.11 | −13.1 ± 0.2 | <0.08 | 12.1 ± 7.1 | >0.9 |
HD 217086 | 36.8 ± 1.1 | 3.88 ± 0.11 | −14.2 ± 1.3 | 0,13 ± 0.07 | >5.0 | > 0.8 |
HD 149757 | 32.5 ± 1.6 | 3.52 ± 0.22 | <−13.3 | 0.13 ± 0.07 | >9.4 | <1.3 |
HD 190864 | 37.5 ± 1.0 | 3.85 ± 0.10 | −12.9 ± 0.1 | >0.16 | >11.8 | > 1.1 |
HD 203064 | 35.6 ± 0.9 | 3.87 ± 0.06 | −12.8 ± 0.1 | 0.15 ± 0.05 | >8.4 | >1.2 |
HD 15570 | 39.1 ± 0.3 | 3.52 ± 0.03 | −12.4 ± 0.1 | <0.08 | <19.9 | 1.1 ± 0.1 |
HD 14947 | 41.9 ± 1.0 | >3.94 | −12.6 ± 0.1 | > 0.15 | >5.0 | >1.1 |
HD 30614 | 28.5 ± 0.6 | <2.90 | −12.7 ± 0.1 | <0.09 | >10.1 | 1.0 ± 0.2 |
HD 210809 | 34.6 ± 1.3 | >3.43 | −12.6 ± 0.1 | >0.08 | >5.0 | >0.8 |
HD 209975 | 32.5 ± 1.0 | 3.39 ± 0.13 | <−13.6 | 0.15 ± 0.05 | >14.8 | >0.8 |
Notes. For upper and lower limits see caption of Table 10.
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