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Table 4

Absolute s-process element abundances A(X) (defined as A(X) = log  [n(X) /n(H)] + 12, where n(X) and n(H) are the number densities of X and H).

Star A(Sr) A(Y) A(Zr) A(Ba) A(La) A(Ce)

V1261 Ori 2.66 ± 0.27 (3) 3.48 ± 0.17 (4) 3.02 ± 0.32 (3) 1.91 ± 0.06 (2) 2.33 ± 0.07 (7)
IT Vir 3.44 ± − (1) 2.70 ± 0.12 (3) 3.99 ± 0.26 (7) 4.05 ± 0.18 (3) 2.42 ± 0.23 (4) 2.52 ± 0.20 (8)
56 Peg 3.05 ± 0.06 (2) 2.22 ± 0.22 (8) 2.44 ± 0.07 (7) 3.18 ± 0.18 (3) 1.12 ± 0.09 (8) 1.41 ± 0.09 (6)
DR Dra 3.04 ± 0.05 (2) 2.13 ± 0.22 (5) 2.77 ± 0.06 (5) 2.46 ± 0.08 (4) 1.17 ± 0.10 (8) 1.56 ± 0.07 (4)
ζ Cyg 3.33 ± − (1) 2.61 ± 0.16 (7) 2.96 ± 0.20 (9) 3.16 ± 0.25 (4) 1.52 ± 0.08 (9) 1.87 ± 0.12 (11)
IP Eri 3.14 ± − (1) 2.06 ± 0.12 (9) 2.86 ± 0.20 (7) 2.53 ± 0.09 (3) 1.25 ± 0.17 (6) 1.60 ± 0.09 (4)
V1379 Aql 2.89 ± − (1) 2.23 ± 0.04 (4) 2.59 ± 0.02 (2) 2.29 ± 0.07 (3) 1.11 ± 0.05 (3) 1.52 ± 0.16 (3)
HR5692 3.16 ± − (1) 2.63 ± 0.20 (6) 3.14 ± 0.19 (11) 2.90 ± 0.07 (5) 1.49 ± 0.10 (11) 1.77 ± 0.13 (9)
ζ Cap 3.86 ± 0.06 (2) 3.50 ± 0.21 (9) 3.87 ± 0.28 (11) 4.06 ± 0.13 (3) 2.09 ± 0.10 (11) 2.47 ± 0.15 (10)
63 Eri 2.84 ± 0.01 (2) 2.06 ± 0.13 (10) 2.48 ± 0.17 (8) 2.64 ± 0.22 (4) 1.15 ± 0.06 (10) 1.55 ± 0.06 (9)
14 Aur C 3.04 ± 0.05 (3) 2.03 ± 0.12 (7) 2.64 ± 0.07 (5) 2.60 ± 0.16 (4) 1.22 ± 0.11 (5) 1.50 ± 0.20 (3)

Suna 2.92 ± 0.05 2.21 ± 0.02 2.58 ± 0.02 2.17 ± 0.07 1.13 ± 0.05 1.70 ± 0.10

Notes. Only the statistical uncertainties are given here. The number of lines used are given in parentheses.

(a)

Solar abundances from Grevesse et al. (2007).

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