Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.62-0.2 | +-0.2 | 2.06 |
CH | ... | -2.30+-0.25 | 0.32+-0.25 | 6.33 |
CN | ... | <-0.17 | <2.45 | <7.8 |
O I | ... | <-2.28 | <0.34 | <6.59 |
Mg I | ... | -2.30+-0.21 | 0.32+-0.21 | 5.3 |
Al I | ... | -3.43+-0.3 | -0.81+-0.3 | 3.03 |
Si I | ... | -2.19+-0.36 | 0.43+-0.36 | 5.32 |
Ca I | ... | -2.06+-0.22 | 0.56+-0.22 | 4.28 |
Sc II | ... | -2.60+-0.14 | 0.02+-0.14 | 0.75 |
Ti I | ... | -2.15+-0.2 | 0.47+-0.2 | 2.8 |
Ti II | ... | -2.34+-0.15 | 0.28+-0.15 | 2.81 |
V II | ... | <-1.78 | <0.84 | <2.22 |
Cr I | ... | -2.77+-0.23 | -0.15+-0.23 | 2.88 |
Mn I | ... | -3.06+-0.2 | -0.44+-0.2 | 2.37 |
Fe I | ... | -2.62+-0.22 | ... | 4.88 |
Fe II | ... | -2.42+-0.14 | ... | 5.08 |
Co I | ... | -2.57+-0.23 | 0.05+-0.23 | 2.43 |
Ni I | ... | -2.63+-0.26 | -0.01+-0.26 | 3.59 |
Zn I | ... | <-1.79 | <0.83 | <2.81 |
Rb I | ... | <0.41 | <3.03 | <3.01 |
Sr II | ... | -2.49+-0.24 | 0.13+-0.24 | 0.58 |
Y II | ... | -2.74+-0.17 | -0.12+-0.17 | -0.33 |
Zr II | ... | -2.15+-0.15 | 0.47+-0.15 | 0.63 |
Nb II | ... | <0.40 | <3.02 | <1.82 |
Mo I | ... | <-0.24 | <2.38 | <1.68 |
Tc I | ... | <1.83 | <4.45 | <1.83 |
Ba II | ... | -2.62+-0.15 | 0.00+-0.15 | -0.24 |
La II | ... | <-1.33 | <1.29 | <-0.16 |
Ce II | ... | <-1.03 | <1.59 | <0.55 |
Pr II | ... | <-0.51 | <2.11 | <0.2 |
Nd II | ... | <-1.13 | <1.49 | <0.37 |
Sm II | ... | <-0.65 | <1.97 | <0.36 |
Eu II | ... | -1.62+-0.18 | 1+-0.18 | -0.9 |
Gd II | ... | <-0.52 | <2.10 | <0.6 |
Tb II | ... | <0.15 | <2.77 | <0.05 |
Dy II | ... | <-1.03 | <1.59 | <0.11 |
Er II | ... | <-0.67 | <1.95 | <0.26 |
Tm II | ... | <-0.14 | <2.48 | <-0.14 |
Yb II | ... | -1.69+-0.17 | 0.93+-0.17 | -0.57 |
Hf II | ... | <0.22 | <2.84 | <1.1 |
Pb I | ... | <-0.05 | <2.57 | <1.9 |
Th II | ... | <0.10 | <2.72 | <0.1 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)