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Issue A&A
Volume 453, Number 1, July I 2006
Page(s) L5 - L8
Section Letters
DOI http://dx.doi.org/10.1051/0004-6361:20065157



A&A 453, L5-L8 (2006)
DOI: 10.1051/0004-6361:20065157

Letter

Coma revealed as an extended hard X-rays source by INTEGRAL IBIS/ISGRI

M. Renaud1, 2, G. Bélanger1, 2, J. Paul1, 2, F. Lebrun1, 2 and R. Terrier2

1  Service d'Astrophysique, CEA-Saclay, 91191 Gif-Sur-Yvette, France
    e-mail: mrenaud@cea.fr
2  APC-UMR 7164, 11 place M. Berthelot, 75231 Paris, France

(Received 7 March 2006 / Accepted 26 April 2006)

Abstract
Aims.We report the INTEGRAL/IBISobservations of the Coma Clusterin the hard X-ray/soft $\gamma$-raydomain.
Methods.Since the Coma Clusterappears as an extended source, its global intensity and significance cannot be directly extracted with standard coded mask analysis. We used the method of imaging the extended sources with a coded mask telescope developed by Renaud et al. (2006).
Results.The imaging capabilities and the sensitivity of the IBIS/ISGRIcoded mask instrument allows us to identify for the first time the site of the emission above ~15 keV. We have studied the Coma Clustermorphology in the 18-30 keV band and found that it follows the prediction based on X-rayobservations. We also bring constraints on the non-thermal mechanism contribution at higher energies.


Key words: galaxies: clusters: Coma Cluster -- methods: data analysis -- gamma rays: observations -- X-rays: galaxies: clusters



© ESO 2006


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