Pulsar Wind Nebulae from X-rays to VHE gamma-rays
High Energy Astrophysical Phenomena
2012-07-09 v1
Abstract
The number of plausible associations of extended VHE (TeV) sources with pulsars has been steadily growing, suggesting that many of these sources are pulsar wind nebulae (PWNe). Here we overview the recent progress in X-ray and TeV observations of PWNe and summarize their properties.
Keywords
Cite
@article{arxiv.1207.1681,
title = {Pulsar Wind Nebulae from X-rays to VHE gamma-rays},
author = {Oleg Kargaltsev and George G. Pavlov and Martin Durant},
journal= {arXiv preprint arXiv:1207.1681},
year = {2012}
}
Comments
8 pages, 6 figures; to appear in the proceedings of the "Electromagnetic Radiation from Pulsars and Magnetars" conference, April 24-27, 2012, Zielona Gora, Poland