Fig. 8.

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Values of the offset of the central galaxy from the optical luminosity weighted centre for each member of the X-ray overluminous (blue), X-ray normal (black), and X-ray underluminous (red) sub-samples. Underluminous groups with X-ray upper limits are denoted with a light red triangle. The main panel shows the values for each group, while the right panel shows the distribution of central galaxy offset for each of the sub-samples. The top panel shows the sub-sample means, both across the full range in Lopt (stars) and split into two bins in Lopt (circles). X-ray underluminous systems have, on average, larger offsets than the X-ray overluminous groups.
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