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arXiv · 1002.0885

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

Oleg Kargaltsev·George Pavlov
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Abstract

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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Oleg Kargaltsev, George Pavlov. 2010-04-09. Pulsar-wind nebulae in X-rays and TeV gamma-rays. https://doi.org/10.1063/1.3475228

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