Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <-0.03 | <2.29 | <1.13 |
CH | ... | -1.29+-0.25 | 1.03+-0.25 | 7.14 |
CN | ... | <-0.86 | <1.46 | <7.11 |
O I | ... | -1.68+-0.16 | 0.64+-0.16 | 7.01 |
Na I | ... | -1.98+-0.28 | 0.34+-0.28 | 4.26 |
Mg I | ... | -1.84+-0.17 | 0.48+-0.17 | 5.76 |
Al I | ... | -2.96+-0.27 | -0.64+-0.27 | 3.49 |
K I | ... | -2.04+-0.2 | 0.28+-0.2 | 2.99 |
Ca I | ... | -1.84+-0.19 | 0.48+-0.19 | 4.5 |
Sc II | ... | -2.26+-0.14 | 0.06+-0.14 | 0.88 |
Ti I | ... | -2.07+-0.17 | 0.25+-0.17 | 2.89 |
Ti II | ... | -2.03+-0.15 | 0.29+-0.15 | 2.92 |
V I | ... | -2.23+-0.19 | 0.09+-0.19 | 1.7 |
V II | ... | -2.23+-0.23 | 0.09+-0.23 | 1.7 |
Cr I | ... | -2.41+-0.17 | -0.09+-0.17 | 3.23 |
Cr II | ... | -2.03+-0.15 | 0.29+-0.15 | 3.61 |
Mn I | ... | -2.62+-0.17 | -0.3+-0.17 | 2.82 |
Fe I | ... | -2.32+-0.17 | ... | 5.18 |
Fe II | ... | -2.32+-0.15 | ... | 5.18 |
Co I | ... | -2.37+-0.2 | -0.05+-0.2 | 2.62 |
Ni I | ... | -2.31+-0.21 | 0.01+-0.21 | 3.91 |
Zn I | ... | -1.97+-0.17 | 0.35+-0.17 | 2.59 |
Rb I | ... | <-0.09 | <2.23 | <2.51 |
Sr II | ... | -1.61+-0.22 | 0.71+-0.22 | 1.26 |
Y II | ... | -2.24+-0.15 | 0.08+-0.15 | -0.03 |
Zr II | ... | -1.95+-0.15 | 0.37+-0.15 | 0.63 |
Nb II | ... | <-0.53 | <1.79 | <0.89 |
Mo I | ... | <-0.94 | <1.38 | <0.98 |
Tc I | ... | <1.19 | <3.51 | <1.19 |
Ba II | ... | -0.94+-0.18 | 1.38+-0.18 | 1.24 |
La II | ... | -1.48+-0.15 | 0.84+-0.15 | -0.38 |
Ce II | ... | -1.35+-0.15 | 0.97+-0.15 | 0.22 |
Pr II | ... | -1.48+-0.15 | 0.84+-0.15 | -0.76 |
Nd II | ... | -1.40+-0.15 | 0.92+-0.15 | 0.01 |
Sm II | ... | -1.75+-0.15 | 0.57+-0.15 | -0.79 |
Eu II | ... | -2.08+-0.16 | 0.24+-0.16 | -1.56 |
Tb II | ... | <-0.24 | <2.08 | <-0.34 |
Dy II | ... | -1.74+-0.16 | 0.58+-0.16 | -0.64 |
Er II | ... | -1.63+-0.17 | 0.69+-0.17 | -0.71 |
Tm II | ... | <-0.55 | <1.77 | <-0.55 |
Yb II | ... | -1.59+-0.18 | 0.73+-0.18 | -0.67 |
Hf II | ... | <-1.28 | <1.04 | <-0.4 |
Pb I | ... | -0.39+-0.17 | 1.93+-0.17 | 1.65 |
Th II | ... | <-1.04 | <1.28 | <-1.04 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)