Figure 4 from Dark Matter Halo Profiles of Massive Clusters: Theory versus Observations

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 4.

c ₂₀₀– M ₂₀₀ distribution for the relaxed and full halo samples characterized by the ratio of the standard deviation to the mean value of c ₂₀₀. All three redshifts are plotted. Note that σ _c/ c shows no redshift evolution. The case of Δ = Δ _vir shows identical behavior.

Other Images in This Article

Copyright and Terms & Conditions