Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.91-0.15 | +-0.15 | 0.71 |
CH | ... | -3.56+-0.25 | 0.35+-0.25 | 4.99 |
CN | ... | <-1.82 | <2.09 | <6.15 |
O I | ... | <-1.94 | <1.97 | <6.93 |
Mg I | ... | -3.19+-0.16 | 0.72+-0.16 | 4.41 |
Al I | ... | -4.66+-0.2 | -0.75+-0.2 | 1.79 |
Si I | ... | -3.38+-0.33 | 0.53+-0.33 | 4.13 |
Ca I | ... | -3.55+-0.18 | 0.36+-0.18 | 2.78 |
Sc II | ... | -3.77+-0.15 | 0.14+-0.15 | -0.49 |
Ti I | ... | -3.61+-0.16 | 0.3+-0.16 | 1.34 |
Ti II | ... | -3.96+-0.15 | -0.05+-0.15 | 1.12 |
V II | ... | <-3.35 | <0.56 | <0.65 |
Cr I | ... | -4.26+-0.14 | -0.35+-0.14 | 1.38 |
Mn I | ... | -4.61+-0.14 | -0.7+-0.14 | 0.82 |
Mn II | ... | -4.84+-0.22 | -0.93+-0.22 | 0.72 |
Fe I | ... | -3.91+-0.15 | ... | 3.59 |
Fe II | ... | -3.78+-0.16 | ... | 3.72 |
Co I | ... | -3.79+-0.18 | 0.12+-0.18 | 1.2 |
Ni I | ... | -3.96+-0.18 | -0.05+-0.18 | 2.26 |
Zn I | ... | <-2.85 | <1.06 | <1.75 |
Rb I | ... | <-0.61 | <3.30 | <1.99 |
Sr II | ... | -6.03+-0.16 | -2.12+-0.16 | -3.04 |
Y II | ... | <-4.57 | <-0.66 | <-2.33 |
Zr II | ... | <-3.68 | <0.23 | <-1.08 |
Nb II | ... | <-1.03 | <2.88 | <0.39 |
Mo I | ... | <-2.22 | <1.69 | <-0.3 |
Tc I | ... | <0.00 | <3.91 | <0 |
Ba II | ... | -5.63+-0.17 | -1.72+-0.17 | -3.32 |
Ce II | ... | <-3.07 | <0.84 | <-1.49 |
Pr II | ... | <-2.56 | <1.35 | <-1.85 |
Nd II | ... | <-3.36 | <0.55 | <-1.86 |
Sm II | ... | <-2.54 | <1.37 | <-1.53 |
Eu II | ... | <-3.35 | <0.56 | <-2.84 |
Gd II | ... | <-2.28 | <1.63 | <-1.16 |
Tb II | ... | <-1.73 | <2.18 | <-1.83 |
Dy II | ... | <-3.07 | <0.84 | <-1.93 |
Ho II | ... | <-2.29 | <1.62 | <-2.03 |
Er II | ... | <-2.63 | <1.28 | <-1.7 |
Tm II | ... | <-2.11 | <1.80 | <-2.11 |
Hf II | ... | <-1.87 | <2.04 | <-0.99 |
Pb I | ... | <-1.40 | <2.51 | <0.55 |
Th II | ... | <-1.87 | <2.04 | <-1.87 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)