Dark matter interpretation of the origin of non-thermal phenomena in galaxy clusters

Astronomy and Astrophysics

Volumn 527, Issue 10, 2011, Pages

  Colafrancesco, S ^a,b   Lieu, R ^c   Marchegiani, P ^d   Pato, M ^e,f,g   Pieri, L ^e,h   Buonanno, R ⁱ  

^a INAF OAR   (Italy)

^b ASI   (Italy)

^c UNIVERSITY OF ALABAMA IN HUNTSVILLE   (United States)

^d UNIVERSITÀ DI ROMA LA SAPIENZA   (Italy)

^e UNIVERSITY OF PADOVA   (Italy)

^f INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^g UNIVERSITÉ PARIS DESCARTES   (France)

^h SEZIONE DI PADOVA   (Italy)

ⁱ UNIVERSITY OF ROME TOR VERGATA   (Italy)

Author keywords

cosmology: theory; dark matter; galaxies: clusters: general; galaxies: clusters: individual: Coma

Indexed keywords

CENTRAL MAGNETIC FIELD; COOLING RATES; COSMOLOGY: THEORY; DARK MATTER; DENSITY PROFILE; GALAXIES: CLUSTERS: GENERAL; GALAXIES: CLUSTERS: INDIVIDUAL: COMA; GALAXY CLUSTERS; GAMMA-RAY OBSERVATIONS; GAS COOLING; INTRA-CLUSTER; MULTI FREQUENCY; NEUTRALINO ANNIHILATION; NEUTRALINO MASS; NON-THERMAL RADIATION; NONTHERMAL; NONTHERMAL EMISSION; PHYSICAL EFFECTS; RADIO HALO; SECONDARY PARTICLES; SOFT X-RAY; SPECTRAL ENERGY DISTRIBUTION; UPPER LIMITS;

COOLING; GAMMA RAYS; MAGNETIC FIELDS; MODELS; SPECTROSCOPY; THERMOELECTRICITY;

GALAXIES;

EID: 79551548516     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014738     Document Type: Article

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