Schedule Feb 09, 2006
Very High Energy Emissions from SNRs
Felix Aharonian (MPI, Heidelberg)

I will review the recent observations of multi-TeV gamma-rays from young shell type supernova remnants, and argue that TeV gamma ray emission is produced through interactions of protons accelerated in the shell up toenergies $E \geq$ 100 TeV. I also will discus the high energy signatures, as well as possible observational strategies for the search for GalacticPeVatrons.

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