Where does the hard X-ray diffuse emission in clusters of galaxies come from?

Astronomy and Astrophysics

Volumn 443, Issue 1, 2005, Pages 1-10

  Colafrancesco, S ^a   Marchegiani, P ^b   Perola, G C ^a,b  

^a INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^b SAPIENZA UNIVERSITY OF ROME   (Italy)

Author keywords

Cosmology: diffuse radiation; Cosmology: theory; Galaxies: clusters: general; Radiation mechanisms: non thermal

Indexed keywords

ASTROPHYSICS; CARRIER CONCENTRATION; COMPUTER SIMULATION; DIFFUSION; GALAXIES; HYDRODYNAMICS; LIGHT EMISSION; LIGHT SCATTERING; MAGNETIC FIELDS; MATHEMATICAL MODELS; RELATIVITY; SYNCHROTRON RADIATION;

COSMOLOGY: DIFFUSE RADIATION; COSMOLOGY: THEORY; GALAXIES: CLUSTERS: GENERAL; RADIATION MECHANISMS: NON-THERMAL;

X RAY ANALYSIS;

EID: 27844540457     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20042077     Document Type: Article

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