Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.14-0.2 | +-0.2 | 1.99 |
CH | ... | -1.91+-0.25 | 0.23+-0.25 | 6.32 |
Mg I | ... | -1.83+-0.24 | 0.31+-0.24 | 5.77 |
Al I | ... | -2.91+-0.36 | -0.77+-0.36 | 3.54 |
Si I | ... | -1.70+-0.28 | 0.44+-0.28 | 5.81 |
Ca I | ... | -1.84+-0.23 | 0.3+-0.23 | 4.5 |
Sc II | ... | -2.21+-0.15 | -0.07+-0.15 | 0.74 |
Ti I | ... | -2.01+-0.21 | 0.13+-0.21 | 2.94 |
Ti II | ... | -1.93+-0.15 | 0.21+-0.15 | 2.82 |
V I | ... | -2.24+-0.24 | -0.1+-0.24 | 1.69 |
Cr I | ... | -2.23+-0.21 | -0.09+-0.21 | 3.41 |
Cr II | ... | -1.93+-0.15 | 0.21+-0.15 | 3.51 |
Mn I | ... | -2.39+-0.22 | -0.25+-0.22 | 3.04 |
Fe I | ... | -2.14+-0.21 | ... | 5.36 |
Fe II | ... | -2.34+-0.15 | ... | 5.16 |
Co I | ... | -2.30+-0.29 | -0.16+-0.29 | 2.69 |
Ni I | ... | -1.99+-0.23 | 0.15+-0.23 | 4.23 |
Zn I | ... | <-2.24 | <-0.10 | <2.36 |
Sr II | ... | -2.48+-0.27 | -0.34+-0.27 | 0.19 |
Zr II | ... | -2.00+-0.38 | 0.14+-0.38 | 0.38 |
Ba II | ... | -2.81+-0.16 | -0.67+-0.16 | -0.83 |
Nd II | ... | <-1.40 | <0.74 | <0.1 |
Sm II | ... | <-1.29 | <0.85 | <-0.28 |
Eu II | ... | <-1.51 | <0.63 | <-1 |
Gd II | ... | <-0.90 | <1.24 | <0.22 |
Tb II | ... | <0.39 | <2.53 | <0.29 |
Dy II | ... | <-0.59 | <1.55 | <0.55 |
Pb I | ... | <0.20 | <2.34 | <2.15 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)