Fig. 2.
[O/Fe]–[Fe/H] relation for the ICM and the Galaxy. The ICM Fe abundances and O/Fe abundance ratios (Table 1) are shown as black dots with (statistical) error bars.The Galactic Fe abundances and O/Fe abundance ratios are taken from Israelian et al. (2004; halo, orange), Reddy et al. (2006; disc and halo, cyan), Fabbian et al. (2009; halo, blue), and Nissen et al. (2014; disc and halo, pink).
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