Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <0.42 | <2.83 | <1.58 |
CH | ... | -1.33+-0.25 | 1.08+-0.25 | 7.32 |
NH | ... | <-1.67 | <0.74 | <6.3 |
O I | ... | -1.86+-0.2 | 0.55+-0.2 | 6.83 |
Mg I | ... | -2.08+-0.22 | 0.33+-0.22 | 5.53 |
Al I | ... | -3.10+-0.31 | -0.69+-0.31 | 3.35 |
Si I | ... | -1.79+-0.36 | 0.62+-0.36 | 5.72 |
Ca I | ... | -1.90+-0.22 | 0.51+-0.22 | 4.45 |
Sc II | ... | -2.44+-0.15 | -0.03+-0.15 | 0.93 |
Ti I | ... | -2.05+-0.2 | 0.36+-0.2 | 2.9 |
Ti II | ... | -2.05+-0.14 | 0.36+-0.14 | 3.12 |
V I | ... | -2.24+-0.28 | 0.17+-0.28 | 1.69 |
V II | ... | -2.11+-0.26 | 0.3+-0.26 | 2.04 |
Cr I | ... | -2.53+-0.21 | -0.12+-0.21 | 3.12 |
Cr II | ... | -2.20+-0.14 | 0.21+-0.14 | 3.66 |
Mn I | ... | -2.81+-0.22 | -0.4+-0.22 | 2.62 |
Mn II | ... | -2.97+-0.21 | -0.56+-0.21 | 2.68 |
Fe I | ... | -2.41+-0.21 | ... | 5.09 |
Fe II | ... | -2.19+-0.14 | ... | 5.31 |
Co I | ... | -2.40+-0.24 | 0.01+-0.24 | 2.6 |
Ni I | ... | -2.53+-0.26 | -0.12+-0.26 | 3.69 |
Zn I | ... | -2.14+-0.23 | 0.27+-0.23 | 2.42 |
Rb I | ... | <0.43 | <2.84 | <3.03 |
Sr II | ... | -1.85+-0.22 | 0.56+-0.22 | 1.24 |
Y II | ... | -2.23+-0.17 | 0.18+-0.17 | 0.2 |
Zr II | ... | -1.73+-0.15 | 0.68+-0.15 | 1.07 |
Nb II | ... | <0.06 | <2.47 | <1.48 |
Mo I | ... | <-0.72 | <1.69 | <1.2 |
Tc I | ... | <1.84 | <4.25 | <1.84 |
Ba II | ... | -1.19+-0.14 | 1.22+-0.14 | 1.21 |
La II | ... | -1.36+-0.16 | 1.05+-0.16 | -0.04 |
Ce II | ... | -1.19+-0.18 | 1.22+-0.18 | 0.61 |
Pr II | ... | -1.06+-0.2 | 1.35+-0.2 | -0.12 |
Nd II | ... | -1.27+-0.17 | 1.14+-0.17 | 0.37 |
Sm II | ... | <-0.95 | <1.46 | <0.06 |
Eu II | ... | -1.82+-0.25 | 0.59+-0.25 | -1.08 |
Gd II | ... | <-0.85 | <1.56 | <0.27 |
Tb II | ... | <-0.02 | <2.39 | <-0.12 |
Dy II | ... | -1.35+-0.25 | 1.06+-0.25 | -0.03 |
Tm II | ... | <-0.29 | <2.12 | <-0.29 |
Yb II | ... | -1.40+-0.18 | 1.01+-0.18 | -0.26 |
Hf II | ... | -0.81+-0.27 | 1.6+-0.27 | 0.26 |
Pb I | ... | -0.20+-0.22 | 2.21+-0.22 | 1.84 |
Th II | ... | <-0.24 | <2.17 | <-0.24 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)