Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.99-0.14 | +-0.14 | 1.54 |
CH | ... | -2.94+-0.25 | 0.05+-0.25 | 5.55 |
NH | ... | -2.64+-0.36 | 0.35+-0.36 | 5.25 |
O I | ... | <-2.12 | <0.87 | <6.75 |
Na I | ... | -3.04+-0.27 | -0.05+-0.27 | 3.2 |
Mg I | ... | -2.48+-0.15 | 0.51+-0.15 | 5.12 |
Al I | ... | -3.53+-0.28 | -0.54+-0.28 | 2.92 |
Si I | ... | -2.21+-0.28 | 0.78+-0.28 | 5.3 |
Ca I | ... | -2.49+-0.17 | 0.5+-0.17 | 3.85 |
Sc II | ... | -2.95+-0.15 | 0.04+-0.15 | 0.26 |
Ti I | ... | -2.69+-0.14 | 0.3+-0.14 | 2.26 |
Ti II | ... | -2.80+-0.15 | 0.19+-0.15 | 2.22 |
V II | ... | -2.58+-0.26 | 0.41+-0.26 | 1.41 |
Cr I | ... | -3.18+-0.15 | -0.19+-0.15 | 2.46 |
Cr II | ... | -2.83+-0.17 | 0.16+-0.17 | 2.87 |
Mn I | ... | -3.31+-0.16 | -0.32+-0.16 | 2.12 |
Mn II | ... | -3.41+-0.21 | -0.42+-0.21 | 2.08 |
Fe I | ... | -2.99+-0.15 | ... | 4.51 |
Fe II | ... | -2.93+-0.16 | ... | 4.57 |
Co I | ... | -3.03+-0.18 | -0.04+-0.18 | 1.96 |
Ni I | ... | -2.86+-0.18 | 0.13+-0.18 | 3.36 |
Zn I | ... | <-2.52 | <0.47 | <2.08 |
Rb I | ... | <-0.27 | <2.72 | <2.33 |
Sr II | ... | -3.32+-0.19 | -0.33+-0.19 | -0.39 |
Y II | ... | -3.64+-0.2 | -0.65+-0.2 | -1.37 |
Zr II | ... | -2.93+-0.2 | 0.06+-0.2 | -0.29 |
Nb II | ... | <-0.46 | <2.53 | <0.96 |
Mo I | ... | <-1.48 | <1.51 | <0.44 |
Ba II | ... | -3.76+-0.16 | -0.77+-0.16 | -1.52 |
Ce II | ... | <-2.25 | <0.74 | <-0.67 |
Pr II | ... | <-1.69 | <1.30 | <-0.98 |
Nd II | ... | <-1.80 | <1.19 | <-0.3 |
Sm II | ... | <-1.65 | <1.34 | <-0.64 |
Eu II | ... | <-2.42 | <0.57 | <-1.91 |
Gd II | ... | <-1.33 | <1.66 | <-0.21 |
Tb II | ... | <-0.75 | <2.24 | <-0.85 |
Dy II | ... | <-1.80 | <1.19 | <-0.66 |
Ho II | ... | <-1.26 | <1.73 | <-1 |
Er II | ... | <-1.64 | <1.35 | <-0.71 |
Tm II | ... | <-1.13 | <1.86 | <-1.13 |
Yb II | ... | <-2.49 | <0.50 | <-1.41 |
Hf II | ... | <-0.78 | <2.21 | <0.1 |
Pb I | ... | <-0.82 | <2.17 | <1.13 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)