Neutrino flux predictions for Galactic plerions

Astronomy and Astrophysics – Astrophysics

Scientific paper

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8 pages. Accepted for publication in Astroparticle Physics

Scientific paper

10.1016/S0927-6505(02)00221-9

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 \nu flux at Earth and find that this is
likely to exceed the detection threshold of the upcoming km^2 neutrino
detectors.

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