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Published byIrma van der Heijden Modified over 6 years ago
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High Angular Resolution X-ray and Radio Observations of the Galactic Supernova Remnant G (RX J ) T.G. Pannuti, G. E. Allen, M.D. Filipovic, M. Stupar, P.A. Jones and J. W. Keohane G : a Galactic supernova remnant with an X-ray spectrum dominated by non-thermal emission 75 kilosecond Chandra observation of luminous northwestern rim Fine structure in rim (leading and trailing edges) revealed for first time Estimate of maximum energy of cosmic-ray electrons accelerated along rim: E ≈ 40 TeV
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