The non-thermal X-ray filaments in young Supernova Remnants

Details The non-thermal X-ray filaments in young Supernova Remnants The non-thermal X-ray filaments in young Supernova Remnants

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aps..apr.e1011l&link_type=abstract

American Physical Society, 2009 APS April Meeting, May 2-5, 2009, abstract #E1.011

Physics

Scientific paper

The nature of the non-thermal X-ray filaments in young Supernova Remnants (SNR) is still unclear. In this work we provide simulated spatially resolved emission spectra in the X-ray. We use a one-dimensional diffusion-loss equation to describe the propagation of non-thermal electrons near the shock of a young SNR and to calculate spatially resolved emission spectra in the X-ray. The results suggests that the high-energy electrons are diffused further and hence the width of the radial profile doesn't depend on the observed frequency.

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