2001/10/29 by S. W. Allen, R. W. Schmidt, A. C. Fabian · 22 citations
Physics and Astronomy · #Astrophysics #Astrophysics and Star Formation Studies #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Gravitational lens #Luminosity #Observatory #Physics #Redshift #Scaling #Stellar, planetary, and galactic studies #Virial mass #Virial theorem #Weak gravitational lensing #astro-ph
paper · pdf · doi:10.1046/j.1365-8711.2001.05079.x
published as Mon.Not.Roy.Astron.Soc.328:L37,2001 · 6 pages, 4 figs, 3 tables. Accepted for publication in MNRAS Letters
arxiv created 2001/10/29 · openalex publication_date 2001/12/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We examine the relations linking mass, X-ray temperature and bolometric luminosity for a sample of luminous, relatively relaxed clusters of galaxies observed with the Chandra Observatory, for which independent confirmation of the mass results is available from gravitational lensing studies. Within radii corresponding to a fixed overdensity Δ = 2500 with respect to the critical density at the redshifts of the clusters, the observed temperature profiles, scaled in units of T2500 and r2500, exhibit an approximately universal form which rises within r ∼ 0.3r2500 and then remains approximately constant out to r2500. We obtain best-fitting slopes for the mass–temperature and temperature–luminosity relations consistent with the predictions from simple scaling arguments i.e. and , respectively. We confirm the presence of a systematic offset of ∼40 per cent between the normalizations of the observed and predicted mass–temperature relations for both SCDM and ΛCDM cosmologies.