Fig. 9.
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Stellar, gas, and baryonic mass fractions. Cool-core clusters are shown in blue, and hot-core clusters are shown in orange. Solid lines indicate moving medians, and dashed lines represent 16% and 84% percentiles (2σ) from the Magneticum simulation (Box2b). Observational data is shown in black, with error bars at the 1σ level, based on XMM-Newton, Chandra, and SDSS from Laganá et al. (2013). Left panel: Gas mass fraction inside R2500c. Central panel: Stellar mass fraction inside R2500c. Right panel: Baryonic mass fraction inside R2500c.
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