Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <0.39 | <2.78 | <1.55 |
CH | ... | -0.36+-0.25 | 2.03+-0.25 | 8.25 |
CN | ... | <-1.87 | <0.52 | <6.1 |
O I | ... | -2.03+-0.2 | 0.36+-0.2 | 6.65 |
Mg I | ... | -2.10+-0.23 | 0.29+-0.23 | 5.5 |
Al I | ... | -2.82+-0.33 | -0.43+-0.33 | 3.63 |
Ca I | ... | -2.05+-0.22 | 0.34+-0.22 | 4.29 |
Ti I | ... | -1.90+-0.2 | 0.49+-0.2 | 3.05 |
Ti II | ... | -2.29+-0.14 | 0.1+-0.14 | 2.84 |
V II | ... | -1.73+-0.24 | 0.66+-0.24 | 2.38 |
Cr I | ... | -2.57+-0.19 | -0.18+-0.19 | 3.07 |
Mn I | ... | -2.66+-0.2 | -0.27+-0.2 | 2.77 |
Fe I | ... | -2.39+-0.21 | ... | 5.11 |
Fe II | ... | -2.21+-0.14 | ... | 5.29 |
Ni I | ... | -2.28+-0.22 | 0.11+-0.22 | 3.94 |
Zn I | ... | <-1.76 | <0.63 | <2.84 |
Rb I | ... | <0.13 | <2.52 | <2.73 |
Sr II | ... | -1.51+-0.19 | 0.88+-0.19 | 1.55 |
Y II | ... | -2.01+-0.16 | 0.38+-0.16 | 0.38 |
Zr II | ... | -1.41+-0.14 | 0.98+-0.14 | 1.35 |
Tc I | ... | <2.16 | <4.55 | <2.16 |
Ba II | ... | -0.58+-0.14 | 1.81+-0.14 | 1.78 |
La II | ... | -0.79+-0.14 | 1.6+-0.14 | 0.5 |
Ce II | ... | -0.61+-0.14 | 1.78+-0.14 | 1.15 |
Pr II | ... | -0.57+-0.14 | 1.82+-0.14 | 0.33 |
Nd II | ... | -0.81+-0.14 | 1.58+-0.14 | 0.79 |
Eu II | ... | -1.57+-0.17 | 0.82+-0.17 | -0.87 |
Gd II | ... | <-0.28 | <2.11 | <0.84 |
Tb II | ... | <1.08 | <3.47 | <0.98 |
Dy II | ... | -1.38+-0.23 | 1.01+-0.23 | -0.1 |
Hf II | ... | <0.25 | <2.64 | <1.13 |
Pb I | ... | 0.04+-0.2 | 2.43+-0.2 | 2.08 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)