The dynamical state of A548 from XMM-Newton data: X-ray and radio connection

2008/04/16 by L. Solovyeva, L. P. Solovyeva, S. Anokhin +8 · 1 citation
Mathematics · Physics and Astronomy · #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Cluster (spacecraft) #Computer science #Connection (principal bundle) #Context (archaeology) #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Geology #Geometry #Mathematics #Paleontology #Physics #Pulsars and Gravitational Waves Research #State (computer science) #astro-ph

paper · pdf · doi:10.1051/0004-6361:200809445

A&A, accepted March 20, 2008, (better quality of figures you can look in A&A after publication)

openalex publication_date 2008/04/16 · arxiv created 2008/05/02 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Context. We present a detailed study of the X-ray properties of the galaxy cluster Abell 548b (), using XMM-Newton data, and discuss the connection between the thermal properties and the presence of two extended relic radio sources located at the cluster periphery.

Citations

• Chandraobservation of the multiple merger cluster Abell 521
• Radio relics in a cosmological cluster merger simulation
• Magnetic Field in Clusters of Galaxies

Cited by

• Diffuse radio emission in/around the Coma cluster: beyond simple accretion