Correlation diagram for [Y/Fe] versus [
/Fe] with our data
(full squares), the data of Zhao and Magain (1991) (open circles) and the
data of Nissen and Schuster (1997) (open triangles). Only stars with
[Fe/H] < -0.6 are plotted.
|
Abundance correlations in mildly metal-poor stars Figure 11. |
/Fe] with our data
(full squares), the data of Zhao and Magain (1991) (open circles) and the
data of Nissen and Schuster (1997) (open triangles). Only stars with
[Fe/H] < -0.6 are plotted.