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Table 4

Stellar parameters of the program stars.

# Object T eff log    g ξ vsin   ia ζ a E(B − V) R V b B . C . c log X/H+12d
K cgs km s-1 km s-1 km s-1 mag mag He i C i C ii N i N ii O i O ii Mg i Mg ii
1 HD 12301 12 600 ± 200 2.15 ± 0.10 7 ± 1 10 20 0.48 ± 0.02 3.1 −0.72 11.06 ± 0.06 8.16 ± 0.05 8.12 ± 0.04 8.72 ± 0.06 8.65 ± 0.03
2 HD 12953 9200 ± 200 1.15 ± 0.10 8 ± 1 22 32 0.58 ± 0.02 2.9 −0.13 11.12 ± 0.03 8.40 ± 0.03 8.49
3 HD 13476 8500 ± 150 1.40 ± 0.10 6 ± 1 12 24 0.59 ± 0.02 2.8 0.06 11.16 ± 0.08 8.18 ± 0.12 8.20 ± 0.13 7.44 ± 0.03 7.46 ± 0.04
4 HD 13744 9500 ± 250 1.55 ± 0.15 6 ± 1 12 29 0.76 ± 0.02 3.1 −0.15 11.16 ± 0.05 7.49 ± 0.04 7.39 ± 0.07
5 HD 14433 9150 ± 150 1.40 ± 0.10 7 ± 1 17 29 0.56 ± 0.02 3.1 −0.07 11.10 ± 0.08 8.25 8.23 ± 0.05 7.49 ± 0.06 7.40 ± 0.04
6 HD 14489 9350 ± 250 1.45 ± 0.15 7 ± 1 13 35 0.38 ± 0.02 3.1 −0.14 11.15 ± 0.04 8.51 ± 0.05 8.54 ± 0.08
7 HD 20041 10 000 ± 200 1.65 ± 0.10 7 ± 1 14 37 0.75 ± 0.03 3.1 −0.22 11.08 ± 0.04 8.25 ± 0.04 8.35 ± 0.04
8 HD 21291 10 800 ± 200 1.65 ± 0.10 7 ± 1 32 33 0.46 ± 0.02 3.1 −0.39 11.11 ± 0.04 8.44 ± 0.04 8.48 ± 0.03
9 HD 39970 10 300 ± 200 1.70 ± 0.10 7 ± 1 2 45 0.43 ± 0.02 3.5 −0.28 11.08 ± 0.05 8.13 ± 0.05 8.22 ± 0.14
10 HD 46300 10 000 ± 200 2.15 ± 0.10 3 ± 1 0 14 0.07 ± 0.02 2.5 −0.22 11.11 ± 0.06 8.43 ± 0.07 8.42
11 HD 186745 12 500 ± 200 1.80 ± 0.10 8 ± 1 22 40 1.01 ± 0.02 2.9 −0.72 11.06 ± 0.05 8.37 ± 0.05 8.33 ± 0.03 8.77 ± 0.01 8.77
12 HD 187983 9300 ± 250 1.60 ± 0.15 7 ± 1 15 29 0.70 ± 0.02 3.0 −0.08 11.08 ± 0.07 8.25 8.31 ± 0.12 7.58 ± 0.04 7.50 ± 0.03
13 HD 197345 8700 ± 150 1.20 ± 0.10 8 ± 1 10 29 0.06 ± 0.02 3.1 0.02 11.19 ± 0.06 8.12 ± 0.06 8.07 ± 0.09 7.50 ± 0.05 7.47 ± 0.05
14 HD 202850 10 800 ± 200 1.85 ± 0.10 6 ± 1 14 35 0.19 ± 0.02 3.1 −0.39 11.20 ± 0.07 8.68 ± 0.04 8.74 ± 0.07
15 HD 207260 8800 ± 150 1.35 ± 0.10 7 ± 1 15 25 0.51 ± 0.02 2.5 0.01 11.17 ± 0.04 8.26 ± 0.07 8.17 ± 0.09 7.51 ± 0.05 7.48 ± 0.02
16 HD 207673 9250 ± 100 1.80 ± 0.10 5 ± 1 1 23 0.44 ± 0.02 3.1 −0.08 11.11 ± 0.10 8.18 8.16 ± 0.11 8.48 ± 0.03 8.45 7.51 ± 0.07 7.44 ± 0.04
17 HD 208501 12 700 ± 200 1.85 ± 0.10 8 ± 1 16 56 0.82 ± 0.02 2.7 −0.76 11.07 ± 0.06 8.25 ± 0.08 8.22 ± 0.07 8.74 8.77 ± 0.01
18 HD 210221 8400 ± 150 1.40 ± 0.10 6 ± 1 0 27 0.40 ± 0.02 2.9 0.08 11.13 ± 0.04 8.24 ± 0.07 8.17 ± 0.01 7.51 ± 0.06 7.48 ± 0.03
19 HD 212593 11 200 ± 200 2.10 ± 0.10 5 ± 1 6 24 0.17 ± 0.02 2.8 −0.46 11.15 ± 0.06 8.45 ± 0.02 8.43 ± 0.09
20 HD 213470 8400 ± 150 1.30 ± 0.10 7 ± 1 13 27 0.54 ± 0.03 3.1 0.10 11.08 ± 0.09 7.46 ± 0.03 7.50 ± 0.06
21 BD+602582 11 900 ± 200 1.85 ± 0.10 7 ± 1 35 14 0.85 ± 0.02 3.4 −0.58 11.14 ± 0.07 8.51 ± 0.04 8.56 ± 0.07
22 HD 223960 10 700 ± 200 1.60 ± 0.10 8 ± 1 25 37 0.76 ± 0.02 3.2 −0.37 11.12 ± 0.08 8.57 ± 0.07 8.52
23 HD 195324 9200 ± 150 1.85 ± 0.10 4 ± 1 3 20 0.56 ± 0.02 2.6 −0.07 11.19 ± 0.06 8.11 ± 0.14 8.08 ± 0.06 7.59 ± 0.03 7.54 ± 0.03
24 HD 34085 12 100 ± 150 1.75 ± 0.10 8 ± 1 25 31 0.05 ± 0.02 3.1 −0.65 11.08 ± 0.05 8.50 ± 0.04 8.42 ± 0.05 8.73 ± 0.04 8.76 ± 0.06
25 HD 87737 9600 ± 200 2.05 ± 0.10 4 ± 1 2 17 0.02 ± 0.02 3.1 −0.14 11.17 ± 0.05 8.23 ± 0.10 8.26 ± 0.04 8.54 ± 0.07 8.49 ± 0.06 7.54 ± 0.05 7.52 ± 0.04
26 HD 91533 9100 ± 150 1.50 ± 0.10 6 ± 1 20 29 0.33 ± 0.02 3.5 −0.07 11.15 ± 0.04 8.24 8.15 ± 0.03 7.49 ± 0.12 7.46 ± 0.08
27 HD 111613 9150 ± 150 1.45 ± 0.10 6 ± 1 17 27 0.39 ± 0.03 3.5 −0.08 11.13 ± 0.06 8.21 8.33 ± 0.11 8.46 ± 0.04 8.43 7.54 ± 0.03 7.46 ± 0.04
28 HD 149076 11 100 ± 200 2.05 ± 0.10 5 ± 1 7 37 0.56 ± 0.02 3.5 −0.44 11.14 ± 0.05 8.43 ± 0.09 8.44 ± 0.10 8.78 ± 0.04 8.83
29 HD 149077 9900 ± 150 2.20 ± 0.10 3 ± 1 1 13 0.53 ± 0.03 3.5 −0.20 11.14 ± 0.06 8.48 ± 0.05 8.41 7.58 ± 0.04 7.51 ± 0.04
30 HD 165784 9000 ± 200 1.50 ± 0.10 7 ± 1 18 35 0.86 ± 0.02 3.1 −0.02 11.13 ± 0.03 8.41 8.37 ± 0.05 7.58 ± 0.08 7.54 ± 0.08
31 HD 166167 9600 ± 150 2.00 ± 0.10 4 ± 1 9 20 0.61 ± 0.02 3.5 −0.14 11.09 ± 0.06 7.66 ± 0.07 7.70 ± 0.04
32 HD 80057 9300 ± 150 1.75 ± 0.10 5 ± 1 13 27 0.32 ± 0.02 3.3 −0.09 11.16 ± 0.04 8.22 ± 0.08 8.28 ± 0.13 8.34 ± 0.04 8.29 7.42 ± 0.06 7.40 ± 0.06
33 HD 102878 8900 ± 150 1.50 ± 0.10 6 ± 1 0 35 0.27 ± 0.02 3.4 −0.02 11.15 ± 0.05 8.26 ± 0.12 8.27 ± 0.13 7.50 ± 0.06 7.45 ± 0.06
34 HD 105071 12 000 ± 150 1.85 ± 0.10 7 ± 1 23 39 0.28 ± 0.02 3.7 −0.61 11.13 ± 0.06 8.55 ± 0.06 8.54 ± 0.07 8.78 ± 0.04 8.73 ± 0.09
35 HD 106068 11 600 ± 200 1.90 ± 0.10 6 ± 1 20 45 0.38 ± 0.02 3.4 −0.56 11.13 ± 0.01 8.60 ± 0.04 8.60 ± 0.04 8.75 ± 0.04 8.82 ± 0.04

Notes. 

(a)

Typical uncertainties are  ± 5 km s-1, and  ± 3 km s-1 for the stars with the sharpest lines.

(b)

Typical uncertainties are  ± 0.2.

(c)

Typical uncertainties vary from  ~0.02 mag for the coolest sample stars to  ~0.05 mag for the hottest stars.

(d)

In cases where only one spectral line could be analysed for an ion (no error margin given), a good estimate for the uncertainty is 0.10 dex.

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