Pulsar-wind nebulae in X-rays and TeV gamma-rays - Astrophysics > High Energy Astrophysical PhenomenaReportar como inadecuado




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Abstract: Pulsars are known to be efficient accelerators that produce copious amountsof relativistic particles and inject them into the Galactic medium. Theradiation emitted by such a pulsar wind can be seen from radio throughgamma-rays as a pulsar-wind nebula PWN. Here we overview and summarize recentprogress in X-ray and TeV observations of PWNe.



Autor: Oleg Kargaltsev, George Pavlov

Fuente: https://arxiv.org/



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