On the inverse Compton scattering interpretation of the hard X-ray excesses in galaxy clusters: The case of Ophiuchus

Astronomy and Astrophysics

Volumn 502, Issue 3, 2009, Pages 711-719

  Colafrancesco, S ^a,b   Marchegiani, P ^b,c  

^a ESA ESRIN   (Italy)

^b INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^c UNIVERSITÀ DI ROMA LA SAPIENZA   (Italy)

Author keywords

Cosmology: Theory; Galaxies: Clusters: General; Galaxies: Clusters: Individual: Ophiuchus; Radiation mechanisms: Non thermal

Indexed keywords

CLUSTER CENTERS; COSMIC RAY PROTONS; COSMOLOGY: THEORY; ELECTRON POPULATION; ELECTRON SPECTRUM; GALAXIES: CLUSTERS: GENERAL; GALAXIES: CLUSTERS: INDIVIDUAL: OPHIUCHUS; GALAXY CLUSTERS; HARD X RAY; HIGH-ENERGY ELECTRON; HIGH-ENERGY PARTICLES; INTRA-CLUSTER; INVERSE COMPTON SCATTERING; LOW ENERGIES; MULTI FREQUENCY; NEUTRALINO ANNIHILATION; NEUTRALINOS; PRIMARY ELECTRONS; RADIATION MECHANISMS: NON-THERMAL; RADIO EMISSION; RAY MODELS; SECONDARY ELECTRONS; SPECTRAL ENERGY DISTRIBUTION; SPECTRAL INDICES; VIABLE SOLUTIONS;

AUGER ELECTRON SPECTROSCOPY; COMPTON SCATTERING; COSMIC RAYS; COSMOLOGY; ELECTRONS; EMISSION SPECTROSCOPY; FORECASTING; GALAXIES; GAMMA RAYS; HEATING; INTELLIGENT CONTROL; MAGNETIC FIELDS; SECONDARY EMISSION;

ELECTRON ENERGY LOSS SPECTROSCOPY;

EID: 68649112860     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911843     Document Type: Article

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