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Table 2.

Chemical abundances of ASAS-065 and ASAS-073 and their standard deviations, calculated for elements calculated from more than three spectral parts.

Element Abundances

(Z) ASAS-065 ASAS-073 Solar
C (6) 8.68 ± 0.18(4) 8.57 ± 0.22(5) 8.43
Na (11) 6.57 ± 0.08(6) 6.15 ± 0.09(4) 6.24
Mg (12) 7.71 ± 0.12(4) 7.35 ± 0.09(6) 7.60
Si (14) 7.62 ± 0.26(40) 7.26 ± 0.22(16) 7.51
S (16) 7.27(2) 7.12
Ca (20) 6.57 ± 0.19(31) 6.26 ± 0.10(14) 6.34
Sc (21) 3.37 ± 0.15(25) 2.94 ± 0.06(7) 3.15
Ti (22) 5.14 ± 0.13(148) 4.77 ± 0.17(30) 4.95
V (23) 4.19 ± 0.16(75) 4.01(2) 3.93
Cr (24) 5.79 ± 0.17(147) 5.51 ± 0.16(25) 5.64
Mn (25) 5.55 ± 0.13(50) 5.22 ± 0.17(9) 5.43
Fe (26) 7.59 ± 0.13(387) 7.23 ± 0.08(80) 7.50
Co (27) 5.01 ± 0.17(90) 5.09 ± 0.20(6) 4.99
Ni (28) 6.40 ± 0.17(133) 6.00 ± 0.17(33) 6.22
Cu (29) 4.38 ± 0.21(5) 4.08(1) 4.19
Zn (30) 4.73(2) 4.18(1) 4.56
Sr (38) 2.83(2) 2.85(1) 2.87
Y (39) 2.24 ± 0.19(12) 2.09 ± 0.22(7) 2.21
Zr (40) 2.71 ± 0.33(10) 3.12(1) 2.58
Mo (42) 2.15(2) 1.88
Ru (44) 1.98(1) 1.75
Ba (56) 2.42 ± 0.04(3) 2.39 ± 0.05(3) 2.18
La (57) 1.27 ± 0.24(7) 1.80(2) 1.10
Ce (58) 1.80 ± 0.27(10) 2.29(2) 1.58
Pr (59) 0.46 ± 0.11(3) 0.72
Nd (60) 1.56 ± 0.24(19) 1.59 ± 0.07(3) 1.42
Sm (62) 1.26 ± 0.32(7) 0.96
Eu (63) 1.74(1) 0.52
Tb (65) 0.29(1) 0.30
Dy (66) 0.79(1) 1.10

Notes. Solar values are taken from Asplund et al. (2009). Numbers in parenthesis in Cols. 2 and 3 show the number of individual lines that were used. For less than three lines the uncertainties were not estimated.

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