|
Abundance correlations in mildly metal-poor stars Figure 12. |

/Fe] with our data (full
squares), the data of Edvardsson et al. (1993) for
[Fe/H] > -0.6 (open circles), for [Fe/H] < -0.6 (full
circles) and for the stars also included in our work (full triangles),
joined by dashed lines to their counterparts.