Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -1.93-0.2 | +-0.2 | 2.24 |
CH | ... | -1.66+-0.25 | 0.27+-0.25 | 6.83 |
NH | ... | <-1.07 | <0.86 | <6.9 |
O I | ... | -1.70+-0.2 | 0.23+-0.2 | 6.99 |
Mg I | ... | -1.56+-0.23 | 0.37+-0.23 | 6.04 |
Al I | ... | -2.78+-0.33 | -0.85+-0.33 | 3.67 |
Ca I | ... | -1.52+-0.23 | 0.41+-0.23 | 4.82 |
Sc II | ... | -1.87+-0.14 | 0.06+-0.14 | 1.32 |
Ti I | ... | -1.62+-0.2 | 0.31+-0.2 | 3.33 |
Ti II | ... | -1.57+-0.14 | 0.36+-0.14 | 3.42 |
V I | ... | -1.85+-0.23 | 0.08+-0.23 | 2.08 |
V II | ... | -1.77+-0.25 | 0.16+-0.25 | 2.2 |
Cr I | ... | -2.01+-0.21 | -0.08+-0.21 | 3.63 |
Cr II | ... | -1.73+-0.14 | 0.2+-0.14 | 3.95 |
Mn I | ... | -2.25+-0.21 | -0.32+-0.21 | 3.18 |
Mn II | ... | -2.24+-0.2 | -0.31+-0.2 | 3.23 |
Fe I | ... | -1.93+-0.21 | ... | 5.57 |
Fe II | ... | -1.89+-0.14 | ... | 5.61 |
Co I | ... | -1.99+-0.24 | -0.06+-0.24 | 3 |
Ni I | ... | -1.87+-0.25 | 0.06+-0.25 | 4.35 |
Zn I | ... | -1.79+-0.2 | 0.14+-0.2 | 2.77 |
Rb I | ... | <0.02 | <1.95 | <2.62 |
Sr II | ... | -1.73+-0.22 | 0.2+-0.22 | 1.18 |
Y II | ... | -2.21+-0.17 | -0.28+-0.17 | 0.04 |
Zr II | ... | -1.67+-0.15 | 0.26+-0.15 | 0.95 |
Nb II | ... | <0.18 | <2.11 | <1.6 |
Mo I | ... | <-0.62 | <1.31 | <1.3 |
Tc I | ... | <1.43 | <3.36 | <1.43 |
Ba II | ... | -1.96+-0.14 | -0.03+-0.14 | 0.26 |
La II | ... | -1.56+-0.2 | 0.37+-0.2 | -0.42 |
Ce II | ... | <-1.49 | <0.44 | <0.09 |
Pr II | ... | <-0.70 | <1.23 | <0.01 |
Nd II | ... | <-1.50 | <0.43 | <0 |
Sm II | ... | <-1.01 | <0.92 | <0 |
Eu II | ... | -1.56+-0.22 | 0.37+-0.22 | -1 |
Gd II | ... | <-0.75 | <1.18 | <0.37 |
Tb II | ... | <0.14 | <2.07 | <0.04 |
Dy II | ... | <-1.71 | <0.22 | <-0.57 |
Yb II | ... | -1.76+-0.25 | 0.17+-0.25 | -0.8 |
Hf II | ... | <-0.03 | <1.90 | <0.85 |
Pb I | ... | <0.01 | <1.94 | <1.96 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)