Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <0.53 | <3.65 | <1.69 |
CH | ... | -1.73+-0.25 | 1.39+-0.25 | 6.9 |
CN | ... | <-0.97 | <2.15 | <7 |
Mg I | ... | -2.74+-0.24 | 0.38+-0.24 | 4.85 |
Al I | ... | -3.89+-0.21 | -0.77+-0.21 | 2.56 |
Si I | ... | -2.77+-0.35 | 0.35+-0.35 | 4.74 |
Ca I | ... | -2.62+-0.23 | 0.5+-0.23 | 3.72 |
Sc II | ... | -3.45+-0.14 | -0.33+-0.14 | -0.09 |
Ti II | ... | -3.01+-0.13 | 0.11+-0.13 | 2.15 |
V II | ... | <-1.74 | <1.38 | <2.26 |
Cr I | ... | -3.27+-0.2 | -0.15+-0.2 | 2.36 |
Mn I | ... | -3.53+-0.21 | -0.41+-0.21 | 1.9 |
Fe I | ... | -3.12+-0.22 | ... | 4.38 |
Fe II | ... | -2.91+-0.14 | ... | 4.59 |
Cu I | ... | <-1.42 | <1.70 | <2.79 |
Ga I | ... | <-0.84 | <2.28 | <2.04 |
Sr II | ... | -3.30+-0.17 | -0.18+-0.17 | -0.22 |
Y II | ... | <-1.66 | <1.46 | <0.58 |
Zr II | ... | <-1.80 | <1.32 | <0.8 |
Nb II | ... | <0.44 | <3.56 | <1.86 |
Mo I | ... | <-0.26 | <2.86 | <1.66 |
Tc I | ... | <1.80 | <4.92 | <1.8 |
Ba II | ... | -2.91+-0.14 | 0.21+-0.14 | -0.53 |
La II | ... | <-1.53 | <1.59 | <-0.36 |
Ce II | ... | <-1.11 | <2.01 | <0.47 |
Pr II | ... | <-0.54 | <2.58 | <0.17 |
Nd II | ... | <-1.26 | <1.86 | <0.24 |
Sm II | ... | <-0.63 | <2.49 | <0.38 |
Eu II | ... | <-1.36 | <1.76 | <-0.85 |
Gd II | ... | <-0.47 | <2.65 | <0.65 |
Tb II | ... | <0.31 | <3.43 | <0.21 |
Dy II | ... | <-1.05 | <2.07 | <0.09 |
Ho II | ... | <-0.31 | <2.81 | <-0.05 |
Er II | ... | <-0.61 | <2.51 | <0.32 |
Tm II | ... | <-0.15 | <2.97 | <-0.15 |
Yb II | ... | <-1.50 | <1.62 | <-0.42 |
Hf II | ... | <0.05 | <3.17 | <0.93 |
Pb I | ... | <0.06 | <3.18 | <2.01 |
Th II | ... | <0.20 | <3.32 | <0.2 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)