Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -2.95-0.21 | +-0.21 | 1.65 |
CH | ... | -3.04+-0.25 | -0.09+-0.25 | 5.7 |
NH | ... | <-1.97 | <0.98 | <6 |
Mg I | ... | -2.51+-0.22 | 0.44+-0.22 | 5.08 |
Al I | ... | -3.75+-0.25 | -0.8+-0.25 | 2.69 |
Si I | ... | -2.59+-0.36 | 0.36+-0.36 | 4.92 |
Ca I | ... | -2.41+-0.22 | 0.54+-0.22 | 3.93 |
Sc II | ... | -2.94+-0.15 | 0.01+-0.15 | 0.52 |
Ti I | ... | -2.64+-0.21 | 0.31+-0.21 | 2.31 |
Ti II | ... | -2.77+-0.15 | 0.18+-0.15 | 2.49 |
V II | ... | -2.51+-0.29 | 0.44+-0.29 | 1.73 |
Cr I | ... | -3.11+-0.2 | -0.16+-0.2 | 2.53 |
Cr II | ... | -2.53+-0.15 | 0.42+-0.15 | 3.42 |
Mn I | ... | -3.40+-0.2 | -0.45+-0.2 | 2.02 |
Mn II | ... | -3.38+-0.2 | -0.43+-0.2 | 2.36 |
Fe I | ... | -2.95+-0.21 | ... | 4.55 |
Fe II | ... | -2.64+-0.15 | ... | 4.86 |
Co I | ... | -2.96+-0.23 | -0.01+-0.23 | 2.02 |
Ni I | ... | -3.03+-0.27 | -0.08+-0.27 | 3.19 |
Cu I | ... | <-1.91 | <1.04 | <2.3 |
Sr II | ... | -3.28+-0.19 | -0.33+-0.19 | -0.09 |
Zr II | ... | -2.75+-0.21 | 0.2+-0.21 | 0.14 |
Nb II | ... | <-0.19 | <2.76 | <1.23 |
Mo I | ... | <-0.99 | <1.96 | <0.93 |
Tc I | ... | <1.29 | <4.24 | <1.29 |
Ba II | ... | -4.16+-0.16 | -1.21+-0.16 | -1.67 |
La II | ... | <-1.84 | <1.11 | <-0.67 |
Ce II | ... | <-1.72 | <1.23 | <-0.14 |
Pr II | ... | <-1.18 | <1.77 | <-0.47 |
Nd II | ... | <-1.86 | <1.09 | <-0.36 |
Sm II | ... | <-1.25 | <1.70 | <-0.24 |
Eu II | ... | <-2.04 | <0.91 | <-1.53 |
Gd II | ... | <-0.94 | <2.01 | <0.18 |
Tb II | ... | <-0.37 | <2.58 | <-0.47 |
Dy II | ... | <-1.53 | <1.42 | <-0.39 |
Ho II | ... | <-0.92 | <2.03 | <-0.66 |
Er II | ... | <-1.15 | <1.80 | <-0.22 |
Tm II | ... | <-0.89 | <2.06 | <-0.89 |
Yb II | ... | <-2.59 | <0.36 | <-1.51 |
Hf II | ... | <-0.49 | <2.46 | <0.39 |
Pb I | ... | <-0.42 | <2.53 | <1.53 |
Th II | ... | <-0.65 | <2.30 | <-0.65 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)