Evidence of a Curved Cosmic-Ray Electron Spectrum in the Supernova Remnant SN 1006

Details Evidence of a Curved Cosmic-Ray Electron Spectrum in the Supernova Remnant SN 1006 Evidence of a Curved Cosmic-Ray Electron Spectrum in the Supernova Remnant SN 1006

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.2393a&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

1

Scientific paper

We present the results of a joint spectral analysis of Chandra ACIS X-ray data, some radio data and the CANGAROO gamma-ray data for the eastern rim of the supernova remnant SN 1006. The results provide strong evidence that the shape of the GeV to TeV electron spectrum is curved as has been predicted. The best-fit values of the "maximum" energy of the electrons and the strength of the magnetic field are = 25+10 TeV and b= 10+8 µG, respectively. -7 -5

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