Pulsar Wind Nebulae from X-rays to VHE gamma-rays
  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. 
Oleg Kargaltsev, George G. Pavlov, and Martin Durant
astro-ph.HE