Temperature profiles from cluster simulations overlaid on our results. Light‐shaded band is the same as that in Fig. 7; dark‐shaded band encloses only the scatter of the best‐fit values in Fig. 7. An approximate X‐ray core radius for a 7 keV cluster is marked. Three‐dimensional average profiles for Ω = 1, Ω = 1 + winds, and Ω = 0.2 models are from Evrard et al. (1996); the Ω = 0.3, Λ = 0.7 model is from Eke et al. (1998). The projection effect is shown by the arrow. Also shown are projected profiles from simulations of single clusters from Katz & White (1993) and Bryan & Norman (1997), both for Ω = 1. The latter simulation is Eulerian; all others are Lagrangian.