Acceleration of primary and secondary particles in galaxy clusters by compressible MHD turbulence: From radio haloes to gamma-rays

Monthly Notices of the Royal Astronomical Society

Volumn 410, Issue 1, 2011, Pages 127-142

  Brunetti, G ^a   Lazarian, A ^b  

^a OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^b UNIVERSITY OF WISCONSIN MADISON   (United States)

Author keywords

Acceleration of particles; Galaxies: clusters: general; Radiation mechanisms: non thermal; Radio continuum: general; Turbulence; X rays: general

Indexed keywords

ACCELERATION; GALAXIES; MAGNETOHYDRODYNAMICS; PARTICLE ACCELERATORS; TURBULENCE;

ACCELERATION OF PARTICLES; GALAXIES CLUSTERS; GALAXIES: CLUSTERS: GENERAL; INTERGALACTIC MEDIUM; MAGNETOHYDRODYNAMIC TURBULENCE; RADIATION MECHANISMS: NONTHERMAL; RADIO CONTINUUM: GENERAL; RADIO HALO; SECONDARY PARTICLES; X-RAY GENERAL;

GAMMA RAYS;

EID: 78650114606     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.17457.x     Document Type: Article

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