Fig. 14.
Comparison between the gas mass-weighted abundance measured in this work and the emission-weighted abundance provided by Maughan et al. (2008), for the overlapping 48 clusters. The reference solar abundance for the data points of Maughan et al. (2008) has been adjusted from Anders & Grevesse (1989) to Asplund et al. (2009), for a direct comparison with our results.
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