Studies of Supernova Remnants with VERITAS

Astronomy and Astrophysics – Astronomy

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Scientific paper

The radio and X-ray synchrotron radiation from supernova remnants (SNRs) and a growing collection of dynamical evidence points to the acceleration of cosmic rays at the strong shocks the. Gamma-ray observations of SNRs provide direct access to information about the population of high-energy particles present in SNRs, and in combination with multi-wavelength observations promise to elucidate the nature of the particles (electrons vs. ions), the efficiency of acceleration, and the properties of the confinement, diffusion, and propagation of high-energy particles. This talk will review VERITAS observations of SNRs, including IC 443 and Cassiopeia A, in light of new results from the Fermi Gamma-ray Space Telescope.
This research was supported by grants from the U.S. Department of Energy, the U.S. National Science Foundation and the Smithsonian Institution, by NSERC in Canada, by Science Foundation Ireland and by STFC in the UK.

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