Figure 6
The X-ray luminosity plotted against X-ray temperature for the OWLS simulation. Red stars are the top 30 per cent of clusters in terms of BCG i-band luminosity and blue squares are the bottom 30 per cent. The dashed line is fit to clusters with the most luminous BCGs, the dotted line is fit to those with the least luminous BCGs and the solid line is fit to all.

The X-ray luminosity plotted against X-ray temperature for the OWLS simulation. Red stars are the top 30 per cent of clusters in terms of BCG i-band luminosity and blue squares are the bottom 30 per cent. The dashed line is fit to clusters with the most luminous BCGs, the dotted line is fit to those with the least luminous BCGs and the solid line is fit to all.

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