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

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

2010-02-04

arxiv.org/abs/1002.0885v2

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

8 pages, 1 fugure, 2 tables to appear in the proceedings of "X-ray Astronomy 2009" conference, Bologna, Italy, September, 2009

Scientific paper

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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