IGR J17354–3255 as bench test for investigation of γ-ray emission from Supergiant Fast X-ray Transients

@article{Sguera2013IGRJA,
  title={IGR J17354–3255 as bench test for investigation of γ-ray emission from Supergiant Fast X-ray Transients},
  author={V. Sguera},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2013},
  volume={239},
  pages={76-81}
}
  • V. Sguera
  • Published 2013
  • Physics
  • arXiv: High Energy Astrophysical Phenomena
  • Abstract Among the different types of sources shining in the high energy sky, gamma-ray binaries are rapidly becoming the subject of major interest. In fact, in the last few years a number of High Mass X-ray Binaries (HMXBs) have been firmly detected from MeV to TeV energies, providing secure evidences that particles can be efficiently accelerated up to very high energies in such galactic systems. Similarly to this general and emerging class of gamma-ray binaries, in principle Supergiant Fast X… CONTINUE READING
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