The origin of the diffuse non-thermal X-ray and radio emission in the Ophiuchus cluster of galaxies

Monthly Notices of the Royal Astronomical Society

Volumn 396, Issue 4, 2009, Pages 2237-2248

  Perez Torres M A ^a   Zandanel, F ^a   Guerrero, M A ^a   Pal, S ^b   Profumo, S ^c   Prada, F ^a,d   Panessa, F ^d  

^a INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^b NATIONAL CENTRE FOR RADIO ASTROPHYSICS   (India)

^c UNIVERSITY OF CALIFORNIA SANTA CRUZ   (United States)

^d INAF IASF ROMA   (Italy)

Author keywords

Galaxies: clusters: individual: Ophiuchus; Radiation mechanisms: non thermal

Indexed keywords

COSMIC RAYS; COSMOLOGY; ELECTROMAGNETIC WAVE EMISSION; GALAXIES; GAMMA RAYS; MAGNETIC FIELDS;

CLUSTER OF GALAXIES; GALAXIES: CLUSTERS: INDIVIDUAL: OPHIUCHUS; INTERNATIONAL GAMMA-RAY ASTROPHYSICS LABORATORIES; NONTHERMAL; RADIATION MECHANISMS: NONTHERMAL; RADIO EMISSION; RADIO OBSERVATION; UPPER LIMITS; X-RAY EMISSION; XMM-NEWTON;

X RAY SCATTERING;

EID: 67649890799     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.14883.x     Document Type: Article

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