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Fig. 3


Stellar-to-gas mass ratio within r500 vs. offset between the X-ray flux-weighted center and the BCG position. The symbols have the same meaning as those in Fig. 1. The intrinsic scatter is (41  ±  8)% and (66  ±  11)% for the ten high- and nine low-offset systems, respectively. This indicates that the scatter of the stellar-to-gas mass ratios may reflect the freedom in the formation history of the systems since the last major merging episode.

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