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The artificial broadening of the high-energy end of electron spectrum in supernova remnants

Abstract

Aims.The observed spectrum of a supernova remnant (SNR) is a superposition of many “local” spectra emitted by regions of SNRs that are under different physical conditions. The question remains as to whether the broadening of the high-energy end of the observed nonthermal spectrum of SNRs, like in G347.3-0.

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EDP Sciences OAI-PMH repository (1.2.0)

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Last time updated on 10/04/2020

This paper was published in EDP Sciences OAI-PMH repository (1.2.0).

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