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Table 4

Elemental abundances of Fe and neutron capture elements for the programme and comparison stars.

Star [Fe/H] [Y/Fe] σ n [Zr i/Fe] σ n [Zr ii/Fe] σ n [Ba/Fe] [La/Fe] σ n
HD 967 −0.62 0.06 0.05 4 0.24 0.03 4 0.24 0.00 2 −0.19 0.08 0.05 2
HD 17820 −0.57 −0.04 0.04 4 0.09 ... 1 0.09 0.03 2 −0.10 0.07 0.03 3
HD 107582 −0.62 0.06 0.03 3 −0.05 0.07 2 −0.05 0.07 2 ... 0.07 0.04 2
BD +73 566 a −0.91 0.88 0.10 6 1.02 0.05 4 0.88 0.00 2 1.62 1.21 0.04 3
BD +19 2646 −0.68 −0.12 0.06 3 0.10 0.00 2 0.13 0.00 2 ... 0.08 ... 1
HD 114762 −0.67 −0.03 0.09 4 ... ... ... −0.05 ... 1 −0.10 0.00 0.05 3
HD 117858 −0.55 −0.13 0.10 4 0.12 0.00 3 ... ... ... −0.11 −0.01 0.08 2
BD +13 2698 −0.74 −0.08 0.09 4 0.18 0.04 2 0.18 0.00 2 −0.20 0.10 0.06 2
BD +77 0521 −0.50 −0.12 0.00 3 ... ... ... ... ... ... ... ... ... ...
HD 126512 −0.55 −0.13 0.10 4 0.07 0.00 2 0.07 0.00 2 −0.18 −0.06 0.01 3
HD 131597 −0.64 0.06 0.07 5 0.07 0.05 4 0.09 ... 1 −0.10 0.02 0.09 4
BD +67 925 −0.55 −0.18 0.00 2 0.00 ... 1 ... ... 1 −0.07 ... ... ...
HD 159482 −0.71 −0.11 0.03 4 ... ... ... ... ... ... −0.17 0.05 0.00 3
HD 170737 −0.68 −0.12 0.06 7 −0.03 0.04 7 −0.03 ... 1 ... 0.05 0.01 3
BD +35 3659 b −1.45 −0.12 0.12 3 0.20 ... 1 0.20 ... 1 −0.12 0.20 ... 1
HD 201889 −0.73 0.05 0.05 6 0.21 0.08 3 0.21 ... 1 −0.06 0.04 0.07 4
HD 204521 −0.72 0.01 0.05 6 0.13 0.08 3 0.13 0.00 2 −0.10 0.09 0.01 3
HD 204848 −1.03 0.28 0.08 7 0.38 0.06 7 0.42 0.05 2 0.25 0.25 0.05 4
HD 212029 −0.98 0.18 0.05 4 ... ... ... ... ... ... 0.24 0.22 0.00 3
HD 222794 −0.61 −0.05 0.05 5 0.12 0.06 3 ... ... ... −0.10 0.04 0.02 3
HD 224930 −0.71 0.05 0.05 5 0.13 0.04 2 0.13 ... 1 −0.17 0.07 0.03 3
HD 17548 −0.49 −0.12 0.06 5 0.00 0.00 2 0.00 0.00 1 −0.10 −0.07 0.05 3
HD 150177 −0.50 0.02 0.07 5 0.10 0.09 3 0.06 0.01 2 −0.09 0.03 0.06 3
HD 159307 −0.60 0.05 0.07 2 ... ... ... 0.06 ... 1 −0.08 ... ... ...
HD 165908 −0.52 −0.12 0.06 5 −0.05 0.00 2 −0.05 ... 1 −0.09 0.01 0.06 4
HD 174912 −0.42 −0.12 0.02 4 0.14 0.04 3 0.04 ... 1 −0.07 −0.05 0.03 3
HD 207978 −0.50 −0.04 0.06 4 0.20 0.00 6 0.11 ... 1 −0.10 −0.07 0.00 2
Star [Ce/Fe] σ n [Pr/Fe] σ n [Nd/Fe] σ n [Sm/Fe] σ n [Eu/Fe] σ n
HD 967 −0.02 0.04 2 0.36 0.08 2 0.13 0.05 4 0.32 0.03 3 0.39 0.06 2
HD 17820 0.11 ... 1 0.37 0.00 2 0.14 0.05 5 0.38 0.06 3 0.38 0.07 2
HD 107582 −0.04 0.06 5 0.34 ... 1 0.10 0.05 5 0.28 0.05 3 0.38 0.07 2
BD +73 566 1.25 0.00 3 1.12 0.04 2 1.33 0.07 7 1.00 0.15 3 0.64 0.29 2
BD +19 2646 0.07 0.05 3 0.40 ... 1 0.11 0.04 5 0.22 0.03 3 0.30 ... 1
HD 114762 0.07 0.02 3 0.21 0.01 2 0.07 0.03 4 0.23 0.05 3 0.17 0.11 2
HD 117858 0.15 0.00 3 0.32 0.03 2 −0.04 0.06 4 0.28 0.06 3 0.28 0.01 2
BD +13 2698 −0.05 0.00 2 0.35 ... 1 0.05 0.06 4 0.33 0.07 3 0.31 0.03 2
BD +77 0521 ... ... ... ... ... ... ... ... ... ... ... ... ... ... ...
HD 126512 0.05 0.00 3 0.30 0.00 1 0.03 0.06 5 0.21 0.14 3 0.28 0.02 2
HD 131597 −0.01 0.06 5 0.26 0.02 2 0.13 0.06 7 0.26 0.06 2 0.32 0.03 2
BD +67 925 ... ... ... 0.32 0.04 2 0.08 0.05 6 ... ... ... 0.29 0.07 2
HD 159482 0.05 0.00 2 0.40 ... 1 0.12 0.06 5 0.30 0.06 3 0.33 0.11 2
HD 170737 0.00 0.08 4 0.12 0.03 2 0.14 0.05 7 0.25 0.11 2 0.35 0.03 2
BD +35 3659 ... ... ... ... ... ... 0.25 0.00 3 0.37 ... 1 0.55 ... 1
HD 201889 0.06 0.08 4 0.33 0.05 2 0.06 0.06 6 0.29 0.02 3 0.26 0.09 2
HD 204521 0.06 0.09 2 0.39 0.00 2 0.10 0.05 5 0.30 0.05 3 0.40 0.04 2
HD 204848 0.13 0.13 5 0.24 0.06 2 0.30 0.07 6 0.28 0.06 3 0.27 0.01 2
HD 212029 ... ... ... ... ... ... 0.25 0.09 3 0.50 0.00 2 0.52 0.10 2
HD 222794 0.08 0.05 3 0.40 0.02 2 0.09 0.04 5 0.24 0.06 2 0.37 0.04 2
HD 224930 0.08 0.11 2 0.40 ... 1 0.01 0.02 3 0.31 0.06 3 0.30 0.08 2
HD 17548 0.08 0.03 3 0.21 ... 1 0.01 0.05 4 0.17 0.05 3 0.18 0.06 2
HD 150177 0.05 0.00 2 0.15 ... 1 0.07 0.06 6 0.15 0.02 3 0.20 ... 1
HD 159307 0.05 ... 1 ... ... ... 0.02 0.00 2 0.26 0.04 2 ... ... ...
HD 165908 0.02 0.06 3 0.21 0.01 2 0.02 0.09 6 0.12 0.03 3 0.13 0.07 2
HD 174912 0.07 0.03 3 0.09 0.07 2 0.02 0.07 5 0.17 0.08 3 0.09 0.11 2
HD 207978 0.06 ... 1 ... ... ... 0.10 0.00 3 0.17 0.03 3 0.16 0.04 2

Notes.[Fe/H] are taken from Paper I.

(a)

The star is rich in chemical elements produced by s-and r-processes.

(b)

Probably not a member of Group 3.

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