Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.23-0.21 | +-0.21 | 1.45 |
CH | ... | -2.64+-0.25 | 0.59+-0.25 | 5.65 |
NH | ... | <-1.92 | <1.31 | <6.05 |
Mg I | ... | -2.58+-0.22 | 0.65+-0.22 | 5.03 |
Al I | ... | -3.95+-0.26 | -0.72+-0.26 | 2.5 |
Si I | ... | -2.60+-0.36 | 0.63+-0.36 | 4.91 |
Ca I | ... | -2.79+-0.23 | 0.44+-0.23 | 3.56 |
Sc II | ... | -3.54+-0.14 | -0.31+-0.14 | -0.53 |
Ti I | ... | -2.65+-0.21 | 0.58+-0.21 | 2.3 |
Ti II | ... | -3.08+-0.13 | 0.15+-0.13 | 1.73 |
V II | ... | <-2.14 | <1.09 | <1.86 |
Cr I | ... | -3.45+-0.2 | -0.22+-0.2 | 2.19 |
Mn I | ... | -3.84+-0.2 | -0.61+-0.2 | 1.59 |
Fe I | ... | -3.23+-0.21 | ... | 4.27 |
Fe II | ... | -3.37+-0.15 | ... | 4.13 |
Co I | ... | -3.14+-0.23 | 0.09+-0.23 | 1.85 |
Ni I | ... | -2.95+-0.22 | 0.28+-0.22 | 3.27 |
Zn I | ... | <-1.85 | <1.38 | <2.75 |
Sr II | ... | -3.26+-0.17 | -0.03+-0.17 | -0.53 |
Y II | ... | <-3.05 | <0.18 | <-0.81 |
Zr II | ... | <-2.25 | <0.98 | <0.35 |
Mo I | ... | <-0.62 | <2.61 | <1.3 |
Tc I | ... | <1.40 | <4.63 | <1.4 |
Ba II | ... | -3.59+-0.14 | -0.36+-0.14 | -1.55 |
Ce II | ... | <-1.50 | <1.73 | <0.08 |
Pr II | ... | <-1.04 | <2.19 | <-0.33 |
Nd II | ... | <-1.66 | <1.57 | <-0.16 |
Sm II | ... | <-0.97 | <2.26 | <0.04 |
Eu II | ... | <-1.69 | <1.54 | <-1.18 |
Gd II | ... | <-0.89 | <2.34 | <0.23 |
Tb II | ... | <0.42 | <3.65 | <0.32 |
Dy II | ... | <-1.46 | <1.77 | <-0.32 |
Er II | ... | <-0.88 | <2.35 | <0.05 |
Tm II | ... | <-0.40 | <2.83 | <-0.4 |
Hf II | ... | <-0.28 | <2.95 | <0.6 |
Pb I | ... | <-0.19 | <3.04 | <1.76 |
Th II | ... | <-0.38 | <2.85 | <-0.38 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)