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On the Radial Density Profile of Intracluster Gas Tracing the Isothermal Dark Halo with a Finite Core

  • Authors: Xiang-Ping Wu and Yan-Jie Xue

Wu & Xue 2000 The Astrophysical Journal 542 578.

  • Provider: AAS Journals

Caption: Fig. 4.

Correlations between the slope and scale parameters in the RDH profile and β model determined from the 45 MME clusters. The solid lines show the best‐fit relations.

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