Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -0.16+-0.11 | 3.67+-0.11 | 1+-0.11 |
Be II | ... | <-2.95 | <0.88 | <-1.8 |
CH | ... | -2.48 | 1.35+-0.21 | 5.95+-0.37 |
NH | ... | -3.43 | 0.4+-0.31 | 4.4+-0.44 |
O I | ... | <-1.49 | <+2.34 | <7.20 |
OH | ... | -2.19 | 1.64+-0.25 | 6.5+-0.42 |
Na I | ... | -3.53 | 0.3+-0.1 | 2.71+-0.18 |
Mg I | ... | -3.37 | 0.46+-0.08 | 4.23+-0.21 |
Al I | ... | -4.39 | -0.56+-0.14 | 2.06+-0.2 |
Si I | ... | -3.34 | 0.49+-0.14 | 4.17+-0.26 |
S I | ... | <-2.77 | <+1.06 | <4.35 |
K I | ... | <-3.08 | <+0.75 | <1.95 |
Ca I | ... | -3.52 | 0.31+-0.1 | 2.82+-0.11 |
Ca II | ... | -2.92 | 0.91+-0.15 | 3.42+-0.18 |
Sc II | ... | -3.54 | 0.29+-0.07 | -0.39+-0.18 |
Ti I | ... | -3.47 | 0.36+-0.08 | 1.48+-0.17 |
Ti II | ... | -3.47 | 0.36+-0.08 | 1.48+-0.17 |
V I | ... | <-3.63 | <+0.20 | <0.30 |
V II | ... | -3.85 | -0.02+-0.1 | 0.08+-0.19 |
Cr I | ... | -4.20 | -0.37+-0.07 | 1.44+-0.17 |
Cr II | ... | -4.05 | -0.22+-0.1 | 1.59+-0.16 |
Mn I | ... | -4.94 | -1.11+-0.11 | 0.49+-0.2 |
Mn II | ... | -4.62 | -0.79+-0.08 | 0.81+-0.16 |
Fe I | ... | -3.83 | ... | 3.67+-0.19 |
Fe II | ... | -3.82 | 0.01 | 3.68+-0.15 |
Co I | ... | -3.29 | 0.54+-0.06 | 1.7+-0.2 |
Ni I | ... | -3.75 | 0.08+-0.06 | 2.47+-0.25 |
Cu I | ... | -4.74 | -0.91+-0.11 | -0.55+-0.21 |
Zn I | ... | <-3.66 | <+0.17 | <0.90 |
Sr II | ... | -4.06 | -0.23+-0.12 | -1.19+-0.2 |
Y II | ... | -4.07 | -0.24+-0.15 | -1.86+-0.22 |
Zr II | ... | -3.79 | 0.04+-0.12 | -1.21+-0.2 |
Ba II | ... | -4.43 | -0.60+-0.12 | -2.25+-0.2 |
Eu I | ... | <-3.42 | <+0.41 | <-2.90 |
Pb I | ... | <-1.85 | <+1.98 | <-0.10 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)