Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <0.43 | <3.72 | <1.59 |
CH | ... | -2.94+-0.25 | 0.35+-0.25 | 5.73 |
CN | ... | <-0.27 | <3.02 | <7.7 |
O I | ... | <-2.54 | <0.75 | <6.33 |
Mg I | ... | -2.69+-0.22 | 0.6+-0.22 | 4.91 |
Al I | ... | -3.85+-0.25 | -0.56+-0.25 | 2.61 |
Si I | ... | -2.85+-0.36 | 0.44+-0.36 | 4.66 |
Ca I | ... | -2.65+-0.22 | 0.64+-0.22 | 3.7 |
Sc II | ... | -3.55+-0.15 | -0.26+-0.15 | -0.13 |
Ti I | ... | -2.79+-0.22 | 0.5+-0.22 | 2.17 |
Ti II | ... | -3.02+-0.14 | 0.27+-0.14 | 2.19 |
V II | ... | <-2.31 | <0.98 | <1.69 |
Cr I | ... | -3.43+-0.2 | -0.14+-0.2 | 2.21 |
Mn I | ... | -3.90+-0.22 | -0.61+-0.22 | 1.54 |
Fe I | ... | -3.29+-0.21 | ... | 4.21 |
Fe II | ... | -3.03+-0.15 | ... | 4.47 |
Co I | ... | -3.02+-0.24 | 0.27+-0.24 | 1.97 |
Ni I | ... | -3.37+-0.24 | -0.08+-0.24 | 2.85 |
Zn I | ... | <-2.24 | <1.05 | <2.36 |
Sr II | ... | -3.21+-0.21 | 0.08+-0.21 | -0.08 |
Y II | ... | -3.60+-0.22 | -0.31+-0.22 | -1.13 |
Zr II | ... | -2.83+-0.22 | 0.46+-0.22 | 0.01 |
Mo I | ... | <-0.85 | <2.44 | <1.07 |
Tc I | ... | <1.32 | <4.61 | <1.32 |
Ba II | ... | -4.00+-0.15 | -0.71+-0.15 | -1.56 |
Ce II | ... | <-1.63 | <1.66 | <-0.05 |
Pr II | ... | <-1.08 | <2.21 | <-0.37 |
Nd II | ... | <-1.73 | <1.56 | <-0.23 |
Sm II | ... | <-1.24 | <2.05 | <-0.23 |
Eu II | ... | <-1.92 | <1.37 | <-1.41 |
Gd II | ... | <-1.00 | <2.29 | <0.12 |
Tb II | ... | <-0.21 | <3.08 | <-0.31 |
Dy II | ... | <-1.13 | <2.16 | <0.01 |
Ho II | ... | <-0.94 | <2.35 | <-0.68 |
Er II | ... | <-1.16 | <2.13 | <-0.23 |
Tm II | ... | <-0.70 | <2.59 | <-0.7 |
Yb II | ... | <-2.46 | <0.83 | <-1.38 |
Hf II | ... | <-0.37 | <2.92 | <0.51 |
Pb I | ... | <-0.39 | <2.90 | <1.56 |
Th II | ... | <-0.46 | <2.83 | <-0.46 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)