Figure 6.3. Predicted and observed [X/Fe] versus [Fe/H] for several a- and Fe-peak-elements plus Zn compared with a compilation of data. In particular the black dots are the recent highresolution data from Cayrel et al. (2004). For the other data see references in Francois et al. (2004). The Solar value indicated in the upper right part of each figure is the predicted Solar value for the ratio [X/Fe]. The assumed Solar abundances are those of Grevesse & Sauval (1998) except that for oxygen, for which we take the value of Holweger (2001).

SN II Yields ratios observed/WW95

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