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Supernova remnants (SNRs) are among the strongest candidates to explain theflux of cosmic rays below the knee around 10^15 eV. Pulsar wind nebulae (PWNe),synchrotron nebulae powered by the spin-down of energetic young pulsars,comprise one of the most populous VHE gamma-ray source classes. Gamma-raystudies in the GeV and TeV bands probe the nature (ions vs. electrons),production, and diffusion of high-energy particles in SNRs and PWNe. Forsources that are visible across both the GeV and TeV bands, such as IC 443, thespatial and spectral distribution of gamma rays can be studied over anunprecedented energy range. This presentation will review recent VERITASresults, including studies of Cassiopeia A, IC 443, PSR J1930+1852, and the SNRG106.3+2.7/Boomerang region, and discuss prospects for complementary studies ofSNRs and PWNe in the Fermi and VHE gamma-ray bands.

VERITAS Observations of Supernova Remnants and Pulsar Wind Nebulae in the Fermi Era