Tracing the evolution in the iron content of the intra-cluster medium

2006/09/30 by I. Balestra, P. Tozzi, S. Ettori +6
Mathematics · Physics and Astronomy · #Archaeology #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Cluster (spacecraft) #Computer science #Content (measure theory) #Context (archaeology) #Cover (algebra) #Galaxies: Formation, Evolution, Phenomena #Geography #Mathematics #Physics #Spectral line #Stellar, planetary, and galactic studies #Tracing #astro-ph

paper · pdf · doi:10.1051/0004-6361:20065568

published as A&A 462, 429-442 (2007) · Astronomy and Astrophysics, Volume 462, Issue 2, February I 2007, pp. 429-442

openalex publication_date 2006/11/02 · arxiv created 2007/01/22 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Context.We present a Chandra analysis of the X-ray spectra of 56 clusters of galaxies at , which cover a temperature range of keV.

Citations

• Baryons in Dark Matter Halos
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