• Corpus ID: 119181376

VERITAS Observations of the Vicinity of the Cygnus Cocoon

@article{Weinstein2013VERITASOO,
  title={VERITAS Observations of the Vicinity of the Cygnus Cocoon},
  author={A. Weinstein},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2013}
}
  • A. Weinstein
  • Published 9 March 2013
  • Physics
  • arXiv: High Energy Astrophysical Phenomena
The study of $\gamma$-ray emission from galactic sources such as supernova remnants (SNR) may provide key insights into their potential role as accelerators of cosmic rays up to the knee ($\sim 10^{15}$ eV). The VERITAS Observatory is sensitive to galactic and extragalactic $\gamma$-ray sources in the 100 GeV to 30 TeV energy range. We report here on VERITAS observations of the vicinity of the cocoon of freshly accelerated cosmic rays reported by Fermi, which lies between potential accelerators… 
1 Citations

Figures from this paper

Very Hight Energy Observationa of Shell-Type Supernova Remnants with SHALON Mirror Cherenkov Telescopes

The investigation of VHE gamma-ray sources by any methods, including mirror Cherenkov telescopes, touches on the problem of the cosmic ray origin and, accordingly, the role of the Galaxy in their

References

NNX11AO86G. The Cygnus cocoon contours were graciously provided in electronic form by the Fermi LAT team

  • ApJS,
  • 2010