Detectability of gamma-ray emission from classical novae with Swift/BAT

@article{Senziani2008DetectabilityOG,
  title={Detectability of gamma-ray emission from classical novae with Swift/BAT},
  author={Fabio Senziani and Gerald K. Skinner and Pierre Jean and M L Hernanz},
  journal={Astronomy and Astrophysics},
  year={2008},
  volume={485},
  pages={223-231}
}
Context. Classical novae are expected to emit gamma rays during their explosions. The most important contribution to the early gamma-ray emission comes from the annihilation with electrons of the positrons generated by the decay of 13 Na nd 18 F. The photons are expected to be down-scattered to a few tens of keV, and the emission is predicted to occur some days before the visual discovery and to last∼2 days. Despite a number of attempts, no positive detections of such emission have been made… 

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