Pulsar-wind nebulae in X-rays and TeV gamma-rays

  title={Pulsar-wind nebulae in X-rays and TeV gamma-rays},
  author={Oleg Kargaltsev and George G. Pavlov},
  journal={arXiv: High Energy Astrophysical Phenomena},
Pulsars are known to be efficient accelerators that produce copious amounts of relativistic particles and inject them into the Galactic medium. The radiation emitted by such a pulsar wind can be seen from radio through gamma-rays as a pulsar-wind nebula (PWN). Here we overview and summarize recent progress in X-ray and TeV observations of PWNe. 

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talk at Supernova Remnants and PWNe in the Chandra Era
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