Figure 2 from Dark Matter Halo Profiles of Massive Clusters: Theory versus Observations

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Dark Matter Halo Profiles of Massive Clusters: Theory versus Observations

Authors: Suman Bhattacharya, Salman Habib, Katrin Heitmann, and Alexey Vikhlinin

Bhattacharya et al. 2013 The Astrophysical Journal 766 32.

Provider: AAS Journals

Caption: Figure 2.

c–ν relations at radii r = R ₂₀₀ and r = R _vir for z = 0, 1, and 2, for the relaxed and full samples where ν = δ _c/σ( M _Δ) with δ ~ 1.676, varying only mildly with redshift. The lines are global fits to the data points using a simple assumption for redshift evolution.

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