Xmm-newton and integral analysis of the ophiuchus cluster of galaxies

Astronomy and Astrophysics

Volumn 508, Issue 3, 2009, Pages 1161-1171

  Nevalainen, J ^a   Eckert, D ^b   Kaastra, J ^c   Bonamente, M ^d   Kettula, K ^a  

^a UNIVERSITY OF HELSINKI   (Finland)

^b UNIVERSITÉ DE GENÈVE   (Switzerland)

^c SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^d UNIVERSITY OF ALABAMA IN HUNTSVILLE   (United States)

Author keywords

Galaxies: Clusters: individual: Ophiuchus; Techniques: spectroscopic; X rays: galaxies: clusters

Indexed keywords

BEST-FIT MODELS; CLUSTER OF GALAXIES; COSMIC MICROWAVES; GALAXIES: CLUSTERS: INDIVIDUALS; HADRONIC COLLISIONS; HARD X RAY; HARD X-RAY EMISSION; INTEGRAL ANALYSIS; INVERSE COMPTON SCATTERING; MAGNETIC FIELD STRENGTHS; MOMENTUM SPECTRA; NONTHERMAL; PHOTON INDEX; POWER-LAW COMPONENTS; RELATIVISTIC ELECTRON; SPATIALLY RESOLVED SPECTROSCOPY; THERMAL ELECTRON; THERMAL EMISSIONS; TOTAL EMISSIONS; TOTAL FLUX; X RAYS: GALAXIES: CLUSTERS; XMM-NEWTON; COSMIC MICROWAVE BACKGROUNDS; TECHNIQUES: SPECTROSCOPIC; X-RAYS: GALAXIES: CLUSTERS;

COSMOLOGY; ELECTRONS; GALAXIES; MAGNETIC FIELDS; NUCLEAR ENERGY; PHOTONS; X RAYS;

THERMIONIC EMISSION;

EID: 72849111544     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912542     Document Type: Article

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