AbstractWe performed a joint fit to radio, recent Chandra X-ray, and γ-ray data for the supernova remnant SN 1006 using models of synchrotron and inverse-Compton emission. The results are used to determine the magnetic field strength and the properties of the electron spectrum for the eastern rim of the remnant.


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    Title :

    Fits to X-ray, radio, and TeV data for the eastern rim of SN 1006


    Contributors:
    Allen, G.E (author) / Houck, J.C (author) / Sturner, S.J (author)

    Published in:

    Advances in Space Research ; 33 , 4 ; 440-445


    Publication date :

    2003-07-14


    Size :

    6 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English





    Fits to X-Ray, Radio, and TeV Data for the Eastern Rim of SN 1006

    Allen, G. E. / Houck, J. C. / Sturner, S. J. et al. | British Library Conference Proceedings | 2004


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