Evidence for non-hydrostatic gas from the cluster X-ray to lensing mass ratio

2007/10/31 by A. Mahdavi, H. Hoekstra, Henk Hoekstra +3 · 1 citation
Physics and Astronomy · #Astrophysics and Star Formation Studies #Galaxies: Formation, Evolution, Phenomena #Gamma-ray bursts and supernovae #astro-ph

paper · pdf · doi:10.1111/j.1365-2966.2007.12796.x

8 pages, minor modifications, accepted for publication in MNRAS

arxiv created 2007/12/03 · openalex publication_date 2008/01/31 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

Rich clusters of galaxies host the most massive collapsed dark matter halos. The X-ray emitting intracluster medium (ICM) bound to this halo can be a useful tracer of the dark

Citations

• H I in the Galaxy
• Challenges for Precision Cosmology with X‐Ray and Sunyaev‐Zeldovich Effect Gas Mass Measurements of Galaxy Clusters

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• The Extended Fe Distribution in the Intracluster Medium and the Implications Regarding AGN Heating