Journal
ASTROPARTICLE PHYSICS
Volume 19, Issue 3, Pages 403-407Publisher
ELSEVIER SCIENCE BV
DOI: 10.1016/S0927-6505(02)00221-9
Keywords
high energy photons; neutrinos; supernova remnants
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We consider a class of plerions that have been detected in the TeV range, and investigate the possibility that the emission is due to pi(0) decay. From the TeV flux we derive what is the expected v flux at Earth and find that this is likely to exceed the detection threshold of the upcoming km(2) neutrino detectors. (C) 2002 Elsevier Science B.V. All rights reserved.
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