Figure 17
Surface brightness profile for the southern edge of the subcluster core with the best-fitting projected discontinuity model shown overlaid (solid line). The dashed line corresponds to the best-fitting projected discontinuity model smeared with a Gaussian of width σ= 5 kpc and the dot–dashed line shows the model for the outer cluster emission.

Surface brightness profile for the southern edge of the subcluster core with the best-fitting projected discontinuity model shown overlaid (solid line). The dashed line corresponds to the best-fitting projected discontinuity model smeared with a Gaussian of width σ= 5 kpc and the dot–dashed line shows the model for the outer cluster emission.

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