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Fig. 4

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FFeHeK/F3.5−6 (upper panel; circles) and FFeHK/F3.5−6 (lower panel; triangles) at 0−0.03r180 (red), 0.03−0.06r180 (orange), 0.06−0.1r180 (magenta) 0.1−0.2r180 (green), 0.2−0.3r180 (blue), and 0.3−0.5r180 (black), plotted against the ICM temperature. Closed and open symbols indicate cD clusters and non-cD clusters, respectively. Black solid and dotted lines correspond to the theoretical ratios from the APEC model of FFeHeK/F3.5−6 and FFeHK/F3.5−6, respectively, assuming Fe abundance = 0.3, 0.5, 1.0, 1.5, and 2.0 solar. Here, abundance ratios of elements are assumed to have the solar ratios by Lodders (2003). Those of the MEKAL model assuming Fe abundance = 0.5 solar are plotted as gray lines.

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