In-situ acceleration of subrelativistic electrons in the Coma halo and the halo's influence on the Sunyaev-Zeldovich effect

2006/10/04 by V. A. Dogiel, S. Colafrancesco, C. M. Ko +5 · 5 citations
Physics and Astronomy · #Acceleration #Coma (optics) #Dust and Plasma Wave Phenomena #Electron #Halo #Ionosphere and magnetosphere dynamics #Laser-Plasma Interactions and Diagnostics #Particle acceleration #Plasma #astro-ph

paper · pdf · doi:10.1051/0004-6361:20054092

14 pages, 11 figures, A&A in press

arxiv created 2006/10/04 · openalex publication_date 2006/10/09 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims.The stochastic acceleration of subrelativistic electrons from a background plasma is studied in order to find a possible explanation of the hard X-ray emission detected from the Coma cluster.

Citations

• Is there a hard tail in the Coma Cluster X-ray spectrum?
• Radio Halo and Relic Candidates from the Westerbork Northern Sky Survey
• The non-thermal Sunyaev–Zel'dovich effect in clusters of galaxies
• Nonthermal Hard X‐Ray Emission in Galaxy Clusters Observed with theBeppoSAXPDS
• The Sunyaev–Zel'dovich effect
• Magnetic Field in Clusters of Galaxies

Cited by

• Chandrameasurements of non-thermal-like X-ray emission from massive, merging, radio halo clusters
• X‐Ray Observations of the Coma Cluster in a Broad Energy Band with theINTEGRAL,RXTE, andROSATObservatories
• The Broadband Spectrum of Galaxy Clusters
• On the inverse Compton scattering interpretation of the hard X-ray excesses in galaxy clusters: the case of Ophiuchus
• Origin of Thermal and Non-Thermal Hard X-Ray Emission from the Galactic Center