Simulations of metal enrichment in galaxy clusters by AGN outflows

2006/11/02 by R. Moll, S. Schindler, W. Domainko +6 · 2 citations
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysical Phenomena and Observations #Astrophysics #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Galaxy formation and evolution #Intracluster medium #Materials science #Metal #Metallurgy #Physics #Type-cD galaxy #astro-ph

paper · pdf · doi:10.1051/0004-6361:20066386

published as Astron.Astrophys.463:513-518,2007 · 7 pages, 6 figures, accepted for publication in A&A

arxiv created 2006/11/02 · openalex publication_date 2006/11/23 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims.We assess the importance of AGN outflows with respect to the metal enrichment of the intracluster medium (ICM) in galaxy clusters.

Citations

• Discovery of an Ionized F[CLC]e[/CLC] K Edge in the [ITAL][CLC]z[/CLC][/ITAL] = 3.91 Broad Absorption Line Quasar APM 08279+5255 with [ITAL]XMM-Newton[/ITAL]
• Inhomogeneity in the Hot Intracluster Medium of Abell 1060 Observed with Chandra
• XMM‐NewtonReveals the Quasar Outflow in PG 1115+080
• Simulating the metal enrichment of the intracluster medium
• Overmerging and mass-to-light ratios in phenomenological galaxy formation models
• ChandraTemperature Profiles for a Sample of Nearby Relaxed Galaxy Clusters
• Galactic Winds

Cited by

• Optical variability properties of mini-BAL and NAL quasars
• VLT/X-Shooter Survey of BAL Quasars: Large Distance Scale and AGN Feedback