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Fig. 17

image

Rescaled pressure (top left) and density (top right) profiles considering the azimuthally averaged, ignoring the merger, and ignoring the merging region and considering the M200,t ot and R200,tot required to recover the cosmological gas fraction at the virial radius. We compare these profiles with the Planck envelope (Planck Collaboration Int. V 2013) for pressure, and with the universal density profile (Eckert et al. 2012) for density. Bottom: rescaled entropy and rescaled entropy corrected by the gas mass fraction, before and after correcting for the true total mass.

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