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A&A 414, L41-L44 (2004)
DOI: 10.1051/0004-6361:20031749
Letter
Is there a hard tail in the Coma Cluster X-ray spectrum?
M. Rossetti1, 2 and S. Molendi11 Istituto di Astrofisica Spaziale e Fisica Cosmica, via Bassini 15, 20133 Milano, Italy
2 Università degli Studi di Milano, Dip. di Fisica, via Celoria 16, 20133 Milano, Italy
(Received 30 September 2003 / Accepted 17 December 2003)
Abstract
We report results from a re-analysis of the BeppoSAX observation of Coma and from the
analysis of a second, yet unpublished observation of the same object.
From our re-analysis of the first observation we find that the statistical evidence
for a hard tail is about 2
. From the analysis of the second observation which,
thanks to the lower background and the longer exposure time, is characterized by
a larger signal-to-noise we find no evidence for a hard tail.
From the upper limit on the flux of the hard tail, using the standard Inverse
Compton formulae, we derive a lower limit for the magnetic of
consistent with Faraday rotation measurements.
Key words: cosmic microwave background -- galaxies: clusters: individual: Coma -- magnetic field -- radiation mechanism: non-thermal -- X-rays: galaxies: clusters
Offprint request: M. Rossetti, rossetti@mi.iasf.cnr.it
SIMBAD Objects
© ESO 2004
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