Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <-0.46 | <2.14 | <0.7 |
CH | ... | -2.20+-0.25 | 0.4+-0.25 | 6.21 |
CN | ... | <-2.27 | <0.33 | <5.7 |
O I | ... | <-1.72 | <0.88 | <7.15 |
Mg I | ... | -2.30+-0.14 | 0.3+-0.14 | 5.3 |
Al I | ... | -3.03+-0.21 | -0.43+-0.21 | 3.42 |
K I | ... | -2.52+-0.15 | 0.08+-0.15 | 2.51 |
Ca I | ... | -2.25+-0.14 | 0.35+-0.14 | 4.08 |
Sc II | ... | -2.46+-0.12 | 0.14+-0.12 | 0.67 |
Ti I | ... | -2.37+-0.09 | 0.23+-0.09 | 2.58 |
Ti II | ... | -2.27+-0.12 | 0.33+-0.12 | 2.66 |
V I | ... | -2.46+-0.13 | 0.14+-0.13 | 1.47 |
V II | ... | -2.29+-0.25 | 0.31+-0.25 | 1.62 |
Cr I | ... | -2.62+-0.09 | -0.02+-0.09 | 3.01 |
Cr II | ... | -2.28+-0.17 | 0.32+-0.17 | 3.34 |
Mn I | ... | -3.00+-0.1 | -0.4+-0.1 | 2.42 |
Fe I | ... | -2.6+-0.1 | ... | 4.9 |
Fe II | ... | -2.62+-0.14 | ... | 4.88 |
Co I | ... | -2.67+-0.18 | -0.07+-0.18 | 2.32 |
Ni I | ... | -2.59+-0.16 | 0.01+-0.16 | 3.62 |
Zn I | ... | -2.41+-0.14 | 0.19+-0.14 | 2.15 |
Rb I | ... | <-0.74 | <1.86 | <1.86 |
Sr II | ... | -2.71+-0.1 | -0.11+-0.1 | 0.14 |
Y II | ... | -2.86+-0.16 | -0.26+-0.16 | -0.67 |
Zr II | ... | -2.24+-0.15 | 0.36+-0.15 | 0.32 |
Mo I | ... | <-1.95 | <0.65 | <-0.03 |
Tc I | ... | <0.42 | <3.02 | <0.42 |
Ba II | ... | -3.09+-0.13 | -0.49+-0.13 | -0.93 |
La II | ... | <-2.26 | <0.34 | <-1.09 |
Ce II | ... | <-2.06 | <0.54 | <-0.48 |
Pr II | ... | <-1.16 | <1.44 | <-0.45 |
Sm II | ... | <-1.50 | <1.10 | <-0.49 |
Eu II | ... | <-1.94 | <0.66 | <-1.43 |
Gd II | ... | <-1.24 | <1.36 | <-0.12 |
Tb II | ... | <-0.78 | <1.82 | <-0.88 |
Dy II | ... | <-1.74 | <0.86 | <-0.6 |
Er II | ... | <-1.46 | <1.14 | <-0.53 |
Tm II | ... | <-0.93 | <1.67 | <-0.93 |
Yb II | ... | <-2.16 | <0.44 | <-1.08 |
Hf II | ... | <-0.82 | <1.78 | <0.06 |
Ir I | ... | <-0.60 | <2.00 | <0.75 |
Pb I | ... | <-1.29 | <1.31 | <0.66 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)