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paper

Neutrino flux predictions for Galactic plerions

arXiv:astro-ph/0209537 · doi:10.1016/S0927-6505(02)00221-9

Abstract

We consider a class of plerions that have been detected in the TeV range, and investigate the possibility that the emission is due to π^0 decay. From the TeV flux we derive what is the expected νflux at Earth and find that this is likely to exceed the detection threshold of the upcoming km^2 neutrino detectors.

8 pages. Accepted for publication in Astroparticle Physics