Abundance correlations in mildly metal-poor stars

Figure 12.




Correlation diagram for [Y/Fe] versus [/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.




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