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.
Fits to X-ray, radio, and TeV data for the eastern rim of SN 1006
Advances in Space Research ; 33 , 4 ; 440-445
2003-07-14
6 pages
Article (Journal)
Electronic Resource
English
Fits to X-ray, radio, and TeV data for the eastern rim of SN 1006
Online Contents | 2004
|Fits to X-Ray, Radio, and TeV Data for the Eastern Rim of SN 1006
British Library Conference Proceedings | 2004
|GWLB - Gottfried Wilhelm Leibniz Bibliothek | 1974
Etude technique moteur: Perkins 1006
Automotive engineering | 2003
|