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Fig. 11.

image

Substructure in the WCS footprint. The 15 identified groups are shown in different colours. The background grey contours represent the X-ray emission measured by ROSAT in 0.4−2.4 keV. The dashed grey lines indicate the direction to nearby clusters connected to Coma. The groups identified by Adami et al. (2005) are labelled and denoted by black crosses.

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