Simulating cosmic rays in clusters of galaxies - II. A unified scheme for radio haloes and relics with predictions of the γ-ray emission

Monthly Notices of the Royal Astronomical Society

Volumn 385, Issue 3, 2008, Pages 1211-1241

  Pfrommer, Christoph ^a   Enßlin, Torsten A ^b   Springel, Volker ^b  

^a UNIVERSITY OF TORONTO   (Canada)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Cosmic rays; Galaxies: clusters: general; Large scale structure of Universe; Magnetic fields; Radiation mechanisms: non thermal

Indexed keywords

COSMIC RAYS; COSMOLOGY; ELECTRONS; GALAXIES; GAMMA RAYS; HOT ELECTRONS; RELATIVITY; SHOCK WAVES; SYNCHROTRON RADIATION; SYNCHROTRONS;

'CURRENT; GALAXIES CLUSTERS; GALAXIES: CLUSTERS: GENERAL; LARGE SCALE STRUCTURE OF UNIVERSE; MAGNETIC-FIELD; NON EQUILIBRIUM; RADIATION MECHANISMS: NONTHERMAL; RADIO HALO; STRUCTURE FORMATIONS; SYNCHROTRON EMISSION;

MAGNETIC FIELDS;

EID: 41649096555     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.12956.x     Document Type: Article

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