Very High Energy Emissions from SNRs

Details Very High Energy Emissions from SNRs Very High Energy Emissions from SNRs

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sgrb.confe...1a&link_type=abstract

Presented at the KITP Conference: Supernova and Gamma-Ray Burst Remnants, Feb 9, 2006, Kavli Institute for Theoretical Physics,

Physics

Scientific paper

I will review the recent observations of multi-TeV gamma-rays from youngshell type supernova remnants, and argue that TeV gamma ray emission isproduced through interactions of protons accelerated in the shell up toenergies E ≥ 100 TeV. I also will discus the high energysignatures, as well as possible observational strategies for the search forGalacticPeVatrons.

Affiliated with

Also associated with

No associations

Rating

Very High Energy Emissions from SNRs does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Very High Energy Emissions from SNRs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Very High Energy Emissions from SNRs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1164722