Table 4
Stellar parameters and elemental abundances for our sample of six debris disc-hosting stars.
Element | HD 21997 | 49Ceti | HD 131835 | HD 138813 | HD 110058 | HD 32297 | Sco-Cen | Sun |
---|---|---|---|---|---|---|---|---|
C | −3.48 ± 0.09 | −3.54 ± 0.06 | −3.47 ± 0.05 | −3.56 ± 0.20(*) | −3.61 ± 0.12 | −3.50 ± 0.08 | −3.70 ± 0.19 | −3.57 |
N | −3.83 ± 0.20 | −4.17 ± 0.29 | −4.17 | |||||
O | −3.30 ± 0.11 | −3.12 ± 0.07 | −3.30 ± 0.02 | −3.37 ± 0.03 | −3.49 ± 0.20(*) | −3.31 ± 0.08 | −3.40 ± 0.19 | −3.31 |
Na | – | −5.77 ± 0.20(*) | – | – | – | −6.08 ± 0.20(*) | −5.82 ± 0.25 | −5.76 |
Mg | −4.41 ± 0.11 | −4.39 ± 0.24 | −4.43 ± 0.10 | −4.51 ± 0.10 | −5.34± 0.06 | −4.74 ± 0.14 | −4.51 ± 0.20 | −4.40 |
Al | – | −5.32 ± 0.20(*) | −5.68 ± 0.20(*) | −5.41 ± 0.20(*) | −6.46 ± 0.20(*) | −6.28 ± 0.20(*) | −6.01 ± 0.17 | −5.55 |
Si | −4.39 ± 0.16 | −4.20 ± 0.16 | −4.34 ± 0.10 | – | −5.12± 0.11 | −4.77 ± 0.14 | −4.54 ± 0.33 | −4.49 |
S | −4.97 ± 0.10 | −4.65 ± 0.04 | −4.81 ± 0.01 | – | −5.28 ± 0.11 | −5.24 ± 0.07 | −4.90 ± 0.17 | −4.88 |
Ca | −5.70 ± 0.08 | −5.74 ± 0.11 | −5.68 ± 0.13 | −5.67 ± 0.07 | −6.89 ± 0.06 | −6.02 ± 0.08 | −5.71 ± 0.19 | −5.66 |
Sc | −8.94 ± 0.09 | −8.92 ± 0.08 | −8.96 ± 0.06 | −9.02± 0.13 | −9.59 ± 0.09 | −9.09 ± 0.14 | −9.11 ± 0.25 | −8.85 |
Ti | −7.03 ± 0.17 | −6.97 ± 0.08 | −7.04 ± 0.20 | −7.10± 0.07 | −8.07 ± 0.19 | −7.38 ± 0.11 | −7.22 ± 0.19 | −7.05 |
V | – | – | – | – | −8.51 ± 0.20(*) | −7.96 ± 0.20(*) | −8.35 ± 0.23 | −8.07 |
Cr | −6.29 ± 0.15 | −6.27 ± 0.13 | −6.44 ± 0.21 | −6.33 ± 0.17 | −7.38 ± 0.20 | −6.81 ± 0.11 | −6.41 ± 0.21 | −6.36 |
Mn | −6.63 ± 0.14 | −6.44 ± 0.34 | −6.52 ± 0.18 | – | −7.21 ± 0.08 | −7.13 ± 0.13 | −6.83 ± 0.28 | −6.57 |
Fe | −4.61 ± 0.02 | −4.56 ± 0.01 | −4.54 ± 0.04 | −4.50 ± 0.07 | −5.65 ± 0.06 | −4.99 ± 0.02 | −4.56 ± 0.15 | −4.50 |
Ni | −5.87 ± 0.23 | −5.95 ± 0.16 | −5.80 ± 0.20 | −5.62± 0.06 | −6.52± 0.19 | −6.23 ± 0.04 | −5.97 ± 0.20 | −5.78 |
Cu | −7.59 ± 0.20(*) | – | – | – | −8.20 ± 0.20(*) | −8.02 ± 0.20(*) | −8.28 ± 0.28 | −7.81 |
Zn | −7.56 ± 0.20(*) | −7.65 ± 0.20(*) | – | – | −8.09 ± 0.20(*) | −7.96 ± 0.20(*) | −7.89 ± 0.25 | −7.44 |
Sr | – | – | – | – | −10.21 ± 0.20(*) | – | −9.04 ± 0.34 | −9.13 |
Y | −9.60 ± 0.20 | – | −9.61 ± 0.20(*) | – | −10.41 ± 0.30 | −10.30 ± 0.20(*) | −9.76 ± 0.25 | −9.79 |
Ba | −9.82 ± 0.10 | −9.98 ± 0.11 | −9.88 ± 0.20(*) | −10.08 ± 0.20(*) | −11.16 ± 0.20(*) | −10.07 ± 0.10 | −9.71 ± 0.32 | −9.82 |
La | – | – | – | – | −12.01 ± 0.20(*) | −11.30 ± 0.20(*) | −10.89 ± 1.18 | −10.90 |
Teff | 8440 ± 100 | 8970 ± 100 | 8550 ± 90 | 9300 ± 90 | 7880 ± 80 | 8060 ± 90 | ||
log g | 4.30 ± 0.15 | 4.19 ± 0.15 | 4.15 ± 0.20 | 4.22 ± 0.17 | 4.00 ± 0.05 | 4.25 ± 0.13 | ||
ν sin i | 70.4 ± 0.9 | 196.9 ± 2.1 | 106.2 ± 1.1 | 136.2 ± 1.5 | 154.8 ± 2.8 | 90.1 ± 0.4 | ||
νmic | 2.9 ± 0.4 | 2.5 ± 0.2 | 3.0 ± 0.5 | 2.4 ± 0.3 | 3.0 ± 0.2 | 2.9 ± 0.2 |
Notes. The median abundance of the hot Sco-Cen sample (Table 5) and the Solar abundances are also listed for reference. Abundances are in log(Nel/NH). The (*) mark indicates abundance estimates from a single absorption line, with a typical uncertainty of 0.20 dex assigned. The Sco- Cen column is the median abundance of the hot star sample of Sco-Cen association member stars (right panel of Table 5). The uncertainty is based on the standard deviation of different stellar estimates.
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