Constraining relativistic protons and magnetic fields in galaxy clusters through radio and γ-ray observations: The case of A2256

Astronomy and Astrophysics

Volumn 508, Issue 2, 2009, Pages 599-602

  Brunetti, G ^a  

^a OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

Author keywords

Galaxies: clusters: general; Gamma rays: theory; Radiation mechanisms: non thermal; Radio continuum: general

Indexed keywords

CLUSTER REGIONS; COMPLEMENTARY CONSTRAINTS; CURRENT MODELS; GALAXIES: CLUSTERS: GENERAL; GALAXY CLUSTERS; GAMMA RAYS: THEORY; GHZ FREQUENCIES; HADRONIC MODELS; LARGE POPULATION; PARTICLE ACCELERATION; RADIATION MECHANISMS: NON-THERMAL; RADIO CONTINUUM: GENERAL; RADIO HALO; RELATIVISTIC PARTICLES; SECONDARY PARTICLES; SPECTRAL INDICES; STEEP SPECTRA; SYNCHROTRON EMISSION;

GALAXIES; MAGNETIC FIELDS; PARTICLE ACCELERATOR ACCESSORIES; PROTONS; SYNCHROTRON RADIATION; SYNCHROTRONS;

GAMMA RAYS;

EID: 77955193637     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913177     Document Type: Article

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