Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.00-0.2 | +-0.2 | 1.96 |
CH | ... | -2.96+-0.25 | 0.04+-0.25 | 5.68 |
NH | ... | <-2.02 | <0.98 | <5.95 |
O I | ... | -2.43+-0.23 | 0.57+-0.23 | 6.27 |
Mg I | ... | -2.56+-0.22 | 0.44+-0.22 | 5.04 |
Al I | ... | -3.72+-0.24 | -0.72+-0.24 | 2.73 |
Si I | ... | -2.57+-0.36 | 0.43+-0.36 | 4.94 |
Ca I | ... | -2.44+-0.22 | 0.56+-0.22 | 3.9 |
Sc II | ... | -2.99+-0.16 | 0.01+-0.16 | 0.38 |
Ti I | ... | -2.51+-0.2 | 0.49+-0.2 | 2.45 |
Ti II | ... | -2.60+-0.14 | 0.4+-0.14 | 2.58 |
Cr I | ... | -3.18+-0.2 | -0.18+-0.2 | 2.47 |
Cr II | ... | -2.76+-0.17 | 0.24+-0.17 | 3.1 |
Mn I | ... | -3.50+-0.2 | -0.5+-0.2 | 1.94 |
Mn II | ... | -3.39+-0.23 | -0.39+-0.23 | 2.26 |
Fe I | ... | -3+-0.21 | ... | 4.5 |
Fe II | ... | -2.78+-0.15 | ... | 4.72 |
Co I | ... | -2.90+-0.24 | 0.1+-0.24 | 2.09 |
Ni I | ... | -3.10+-0.27 | -0.1+-0.27 | 3.12 |
Zn I | ... | <-2.33 | <0.67 | <2.27 |
Rb I | ... | <0.07 | <3.07 | <2.67 |
Sr II | ... | -3.07+-0.22 | -0.07+-0.22 | 0.03 |
Y II | ... | -3.25+-0.23 | -0.25+-0.23 | -0.82 |
Zr II | ... | -2.66+-0.18 | 0.34+-0.18 | 0.14 |
Nb II | ... | <0.03 | <3.03 | <1.45 |
Mo I | ... | <-0.95 | <2.05 | <0.97 |
Tc I | ... | <1.33 | <4.33 | <1.33 |
Ba II | ... | -3.63+-0.14 | -0.63+-0.14 | -1.23 |
La II | ... | <-2.07 | <0.93 | <-0.9 |
Ce II | ... | <-1.65 | <1.35 | <-0.07 |
Pr II | ... | <-1.05 | <1.95 | <-0.34 |
Nd II | ... | <-1.72 | <1.28 | <-0.22 |
Sm II | ... | <-1.05 | <1.95 | <-0.04 |
Eu II | ... | <-1.93 | <1.07 | <-1.42 |
Gd II | ... | <-1.09 | <1.91 | <0.03 |
Tb II | ... | <-0.39 | <2.61 | <-0.49 |
Dy II | ... | <-1.34 | <1.66 | <-0.2 |
Ho II | ... | <-0.99 | <2.01 | <-0.73 |
Er II | ... | <-1.28 | <1.72 | <-0.35 |
Tm II | ... | <-0.71 | <2.29 | <-0.71 |
Yb II | ... | <-2.43 | <0.57 | <-1.35 |
Hf II | ... | <-0.55 | <2.45 | <0.33 |
Pb I | ... | <-0.41 | <2.59 | <1.54 |
Th II | ... | <-0.46 | <2.54 | <-0.46 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)