Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.71-0.2 | +-0.2 | 2.11 |
CH | ... | <-1.75 | <0.96 | <6.8 |
NH | ... | <-0.67 | <2.04 | <7.3 |
O I | ... | -2.65+-0.21 | 0.06+-0.21 | 6.04 |
Mg I | ... | -2.33+-0.22 | 0.38+-0.22 | 5.27 |
Al I | ... | -3.55+-0.24 | -0.84+-0.24 | 2.9 |
Si I | ... | -2.54+-0.36 | 0.17+-0.36 | 4.97 |
Ca I | ... | -2.21+-0.23 | 0.5+-0.23 | 4.13 |
Sc II | ... | -2.48+-0.15 | 0.23+-0.15 | 0.58 |
Ti II | ... | -2.16+-0.14 | 0.55+-0.14 | 2.7 |
Cr I | ... | -2.79+-0.2 | -0.08+-0.2 | 2.85 |
Mn I | ... | -3.00+-0.2 | -0.29+-0.2 | 2.43 |
Fe I | ... | -2.71+-0.22 | ... | 4.79 |
Fe II | ... | -2.8+-0.14 | ... | 4.7 |
Co I | ... | -2.70+-0.24 | 0.01+-0.24 | 2.29 |
Ni I | ... | -2.64+-0.23 | 0.07+-0.23 | 3.59 |
Zn I | ... | <-1.94 | <0.77 | <2.66 |
Rb I | ... | <0.19 | <2.90 | <2.79 |
Sr II | ... | -2.74+-0.21 | -0.03+-0.21 | 0.04 |
Y II | ... | -2.65+-0.21 | 0.06+-0.21 | -0.53 |
Mo I | ... | <-0.10 | <2.61 | <1.82 |
Tc I | ... | <2.04 | <4.75 | <2.04 |
Ba II | ... | -3.13+-0.14 | -0.42+-0.14 | -1.04 |
La II | ... | <-1.33 | <1.38 | <-0.16 |
Ce II | ... | <-1.03 | <1.68 | <0.55 |
Pr II | ... | <-0.33 | <2.38 | <0.38 |
Nd II | ... | <-0.91 | <1.80 | <0.59 |
Sm II | ... | <-0.55 | <2.16 | <0.46 |
Eu II | ... | <-1.19 | <1.52 | <-0.68 |
Gd II | ... | <-0.35 | <2.36 | <0.77 |
Tb II | ... | <0.63 | <3.34 | <0.53 |
Dy II | ... | <-1.05 | <1.66 | <0.09 |
Ho II | ... | <-0.15 | <2.56 | <0.11 |
Er II | ... | <-0.52 | <2.19 | <0.41 |
Tm II | ... | <0.08 | <2.79 | <0.08 |
Yb II | ... | <-1.66 | <1.05 | <-0.58 |
Hf II | ... | <0.08 | <2.79 | <0.96 |
Pb I | ... | <0.20 | <2.91 | <2.15 |
Th II | ... | <0.36 | <3.07 | <0.36 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)