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

  • Authors: Yutaka Fujita and Fumio Takahara

Fujita & Takahara 2000 The Astrophysical Journal 536 523.

  • Provider: AAS Journals

Caption: Fig. 1.

Relation between β and ﹩T_{\mathrm{gas}\,}﹩ when ﹩\gamma =1﹩, for ﹩T_{1}=0.5﹩ (dashed line), 1 (solid line), and 2 keV (dotted line. The observational data obtained by Mohr et al. (1999; filled circles) and Peres et al. (1998; open squares) are overlaid.

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