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A novel method for component separation for extended sources in X-ray astronomy. Fabio Acero (CEA Saclay)
A novel method for component separation for extended sources in X-ray astronomy. Fabio Acero (CEA Saclay)
Nov 7 @ 12:00 – 13:00
Supernova remnants (and extended sources in general), are composed of a variety of components from different origins such as the shocked medium, the shocked ejecta or the accelerated electrons. Each component has a spectral signature (bremsstrahlung, emission lines, synchrotron, etc) and a spatial distribution that are projected along the line of sight and the perceived signal is a combination of
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