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Constraints on cosmic-ray origin theories from TeV gamma-ray observations

RW Lessard,IH Bond,SM Bradbury,JH Buckley,AM Burdett,DA Carter-Lewis,M Catanese,MF Cawley,S Dunlea,M D'Vali,DJ Fegan,SJ Fegan,JP Finley,JA Gaidos,T Hall,AM Hillas, DK Horan,J Knapp,F Krennrich,S Le Bohec,C Masterson,J Quinn,HJ Rose,FW Samuelson,GH Sembroski, VV Vassilev,TC Weekes

ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES（1999）

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Abstract
If supernova remnants (SNR) ate the sites of cosmic-ray acceleration, the associated nuclear interactions should result in observable fluxes of TeV gamma-rays from the nearest SNR. A search for gamma-ray emission from six nearby, radio-bright, SNR has been made with the Whipple Observatory's gamma-ray telescope. No significant emission has been detected and upper limits on the >300 GeV flux are reported. Three of these SNR (IC 443, gamma-Cygni and W 44) are spatially coincident with low latitude unidentified sources detected with EGRET.
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