Element | Nline | [X/H] | [X/Fe] | log-e |
Fe I | ... | -2.71+-0.13 | ... | 4.78+-0.13 |
Fe II | ... | -2.70+-0.18 | ... | 4.79+-0.18 |
Sr II | ... | -1.56+-0.16 | +1.15+-0.16 | 1.37+-0.16 |
Y II | ... | -1.79+-0.12 | +0.92+-0.12 | 0.45+-0.12 |
Zr II | ... | -1.40+-0.12 | +1.31+-0.12 | 1.22+-0.12 |
Ba II | ... | 0.03+-0.2 | +2.74+-0.20 | 2.26+-0.20 |
La II | ... | -0.21+-0.13 | +2.50+-0.13 | 1.02+-0.13 |
Ce II | ... | -0.44+-0.12 | +2.27+-0.12 | 1.20+-0.12 |
Pr II | ... | -0.26+-0.12 | +2.45+-0.12 | 0.55+-0.12 |
Nd II | ... | -0.49+-0.12 | +2.22+-0.12 | 1.00+-0.12 |
Sm II | ... | -0.51+-0.12 | +2.20+-0.12 | 0.48+-0.12 |
Eu II | ... | -0.74+-0.2 | +1.97+-0.20 | -0.2+-0.20 |
Gd II | ... | -0.40+-0.13 | +2.31+-0.13 | 0.70+-0.13 |
Dy II | ... | -0.73+-0.2 | +1.98+-0.2 | 0.1+-0.2 |
Er II | ... | -0.67+-0.2 | +2.04+-0.2 | 0.3+-0.2 |
Tm II | ... | -0.75+-0.2 | +1.96+-0.2 | -0.6+-0.2 |
Hf II | ... | 0.05+-0.2 | +2.76+-0.2 | 0.8+-0.2 |
Pb I | ... | -0.06+-0.2 | +2.65+-0.2 | 2.0+-0.2 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)