Table 6: Abundances of cooler stars.
Species   HD 10132 HD 12533 HD 159251
  $\log \epsilon_{\odot}$ [X/H], n, [X/Fe] [X/H], n, [X/Fe] [X/H], n, [X/Fe]

C I		 8.39 $-0.43\pm 0.11, 2,-0.39$ . . . . . .
O I 8.69 -0.20, 1,-0.16 . . . . . .
Na I 6.33 $-0.04\pm 0.19, 4,+0.01$ $+0.14\pm0.16, 2,+0.20$ $-0.10\pm0.03, 2,-0.06$
Mg I 7.58 $-0.18\pm 0.37, 3,-0.14$ -0.24, 1,-0.18 -0.67, 1,-0.63
Al I 6.47 $-0.35\pm0.14, 3,-0.31$ -0.15, 1,-0.09 $-0.21\pm0.09, 2,-0.17$
Si I 7.55 $+0.03\pm0.16,16,+0.08$ $+0.14\pm0.25, 8,+0.20$ $+0.04\pm0.11,20,+0.09$
S I 7.21 $+0.15\pm 0.11, 2,+0.20$ . . . . . .
K I 5.12 . . . +0.21, 1,+0.27 . . .
Ca I 6.36 $+0.05\pm0.20,11,+0.10$ $-0.20\pm0.19,10,-0.14$ $-0.21\pm0.25,25,-0.17$
Sc I 3.10 . . . $-0.12\pm0.16,7,-0.06$ $-0.16\pm0.15,10,-0.11$
Sc II 3.10 $+0.36\pm 0.17, 9,+0.41$ $-0.03\pm0.20, 5,+0.03$ $+0.10\pm0.32, 9,+0.15$
Ti I 4.99 $-0.07\pm0.16,20,-0.03$ $-0.19\pm0.17,38,-0.13$ $-0.13\pm0.21,81,-0.09$
Ti II 4.99 $+0.04\pm0.10, 5,+0.09$ $-0.22\pm0.25, 4,-0.16$ $-0.07\pm0.09, 5,-0.03$
V I 4.00 $-0.05\pm0.24,15,-0.01$ $+0.01\pm0.24,31,+0.07$ $0.03\pm0.20,35,+0.08$
V II 4.00 . . . . . . +0.17, 1,+0.22
Cr I 5.67 $-0.03\pm 0.19,19,+0.02$ $-0.16\pm0.20,22,-0.10$ $-0.07\pm0.22,35,-0.03$
Cr II 5.67 $-0.09\pm0.20,10,-0.05$ $+0.04\pm0.25, 2,+0.10$ $+0.07\pm0.16, 7,+0.12$
Mn I 5.39 $+0.20\pm0.20, 5,+0.25$ $+0.01\pm0.21, 6,+0.07$ $+0.02\pm0.31,16,+0.07$
Fe I 7.52 $-0.01\pm 0.14$,94,....... $-0.08\pm0.18,132,.......$ $-0.03\pm0.16,253,.......$
Fe II 7.52 $-0.08\pm 0.12$,19,....... $-0.04\pm 0.22,11,.......$ $-0.06\pm0.12,18,.......$
Co I 4.92 $-0.07\pm 0.18, 6,-0.03$ $-0.02\pm0.25,11,+0.04$ $+0.17\pm0.24,23,+0.22$
Ni I 6.25 $-0.07\pm0.17,27,-0.03$ $-0.05\pm0.17,38,+0.01$ $-0.04\pm0.24,88,+0.01$
Cu I 4.26 . . . . . . $+0.41\pm0.33,3,+0.46$
Zn I 4.60 $-0.14\pm0.04, 2,-0.10$ -0.05, 1,+0.01 $-0.14\pm0.20,2,-0.09$
Sr I 2.90 . . . . . . -0.21,1,-0.16
Y I 2.24 . . . $-0.24\pm0.16, 2,-0.18$ . . .
Y II 2.24 $-0.05\pm0.13, 4,+0.00$ $-0.12\pm0.15, 3,-0.06$ $-0.06\pm0.21, 3,-0.01$
Zr I 2.60 . . . . . . $-0.10\pm0.12, 6,-0.05$
Zr II 2.60 $+0.12\pm0.04,2,+0.17$ $-0.26\pm0.16, 9,-0.20$ +0.29, 1,+0.34
Mo II 1.92 . . . $+0.04\pm0.10, 2,+0.10$ -0.01, 1,+0.04
Ba II 2.13 $+0.19\pm0.09,2,+0.24$ +0.23, 1, +0.29 $+0.02\pm0.13, 2,+0.07$
La II 1.22 $-0.17\pm0.04, 3,-0.13$ $+0.13\pm0.18, 2,+0.19$ $-0.18\pm0.14, 3,-0.13$
Ce II 1.55 $+0.02\pm0.20, 3,+0.07$ $-0.01\pm0.15, 4,+0.05$ $-0.09\pm0.21, 4,-0.04$
Pr II 0.71 . . . +0.34, 1,+0.40 $+0.16\pm0.10, 2,+0.21$
Nd II 1.50 $-0.11\pm0.17, 6,-0.07$ $0.12\pm0.54, 5,-0.06$ $-0.16\pm0.18, 5,-0.11$
Sm II 1.00 . . . . . . $+0.01\pm0.30, 2,+0.06$
Eu II 0.51 $-0.04\pm0.07, 2,+0.01$ . . . +0.17,1,+0.22


Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 Observations and data reduction
3 Derived elemental abundances
4 Conclusions
References
List of tables
List of figures