Fig. A.2
Radial Fe abundance profiles for all the groups/ellipticals (kTmean< 1.7 keV) in our sample. The radial distances (x-axis) are expressed in fractions of r500 while the Fe abundances (y-axis) are given with respect to their proto-solar values (Lodders et al. 2009). Data points that were not included when computing the average profile were removed (Sect. 4.1).
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