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Consequences of Short‐Range Interactions between Dark Matter and Protons in Galaxy Clusters
Chuzhoy & Nusser 2006 The Astrophysical Journal 645 950.
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.
© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.