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Consequences of Short‐Range Interactions between Dark Matter and Protons in Galaxy Clusters

  • Authors: Leonid Chuzhoy and Adi Nusser

Chuzhoy & Nusser 2006 The Astrophysical Journal 645 950.

  • Provider: AAS Journals

Caption: Fig. 1.

Upper limit on ﹩\sigma _{0}﹩ for ﹩V_{0}=10^{3}﹩ km s−1. The solid and dashed curves correspond to ﹩V_{x}/ V_{p}=1﹩ and 0.1, respectively.

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