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The shape of the cutoff in the synchrotron emission of SN 1006 observed with XMM-Newton | Marco Miceli ( INAF – Osservatorio Astronomico di Palermo)
@ Aula OAPA
The shape of the cutoff in the synchrotron emission of SN 1006 observed with XMM-Newton | Marco Miceli ( INAF – Osservatorio Astronomico di Palermo)
@ Aula OAPA
May 16 @ 15:30 – 16:30
Synchrotron X-ray emission from the rims of young supernova remnants allows us to study the high-energy tail of the electrons accelerated at the shock front. The analysis of X-ray spectra can provide information on the physical mechanisms that limit the energy achieved by the electrons in the acceleration process. We analzsed the deep observations of the XMM-Newton SN 1006 Large
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