Fig. 3 from The Variation of Gas Mass Distribution in Galaxy Clusters: Effects of Preheating and Shocks

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The Variation of Gas Mass Distribution in Galaxy Clusters: Effects of Preheating and Shocks

Fujita & Takahara 2000 The Astrophysical Journal 536 523.

Caption: Fig. 3.

Same as Fig. 2b, but for ﹩\gamma =1.2﹩