@inproceedings{289b30a0d9fc45ec9fade404fb201385,
title = "Pulsar-wind nebulae in X-rays and TeV γ-rays",
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 γ-rays as a pulsar-wind nebula (PWN). Here we overview and summarize recent progress in X-ray and TeV observations of PWNe.",
author = "O. Kargaltsev and Pavlov, \{G. G.\}",
year = "2010",
doi = "10.1063/1.3475228",
language = "English (US)",
isbn = "9780735407954",
series = "AIP Conference Proceedings",
pages = "25--32",
booktitle = "X-ray Astronomy-2009",
note = "International Conference on X-ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future Perspectives ; Conference date: 07-09-2009 Through 11-09-2009",
}