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 Ï^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