Abstract: From radio and higher-frequency observations, more than 300 SNRs have been discovered in the Milky Way, of which 220 fall into the H.E.S.S. Galactic Plane Survey. However only 50 SNRs are coincident with a H.E.S.S source and in 8 cases the VHE emission is firmly associated with the SNR. The H.E.S.S. dataset includes now more than 8 years of observations and it is of great interest to extract VHE flux upper limits from undetected SNRs. These new measurements can then be used to test the standard paradigm of the SNRs as the origin of Galactic cosmic rays. In this contribution, the H.E.S.S. results on the population of SNRs and the subsequent constraints on the cosmic-ray acceleration efficiency in these sources are presented
Abstract: Supernova (SN) remnants are a well motivated candidate for the acceleration sites of cosmi...
Shell-type supernova remnants (SNRs) are considered prime candidates for the acceleration of Galacti...
Abstract: More and more supernova remnants have been revealed to be high energy γ-ray emitters thank...
International audienceShell-type supernova remnants (SNRs) are considered prime candidates for the a...
International audienceSupernova remnants (SNRs) are considered prime candidates for the acceleration...
Abstract: Supernova (SN) remnants are a well motivated candidate for the acceleration sites of cosmi...
Shell-type supernova remnants (SNRs) are considered prime candidates for the acceleration of Galacti...
Abstract: More and more supernova remnants have been revealed to be high energy γ-ray emitters thank...
International audienceShell-type supernova remnants (SNRs) are considered prime candidates for the a...
International audienceSupernova remnants (SNRs) are considered prime candidates for the acceleration...
Abstract: Supernova (SN) remnants are a well motivated candidate for the acceleration sites of cosmi...
Shell-type supernova remnants (SNRs) are considered prime candidates for the acceleration of Galacti...
Abstract: More and more supernova remnants have been revealed to be high energy γ-ray emitters thank...