Pulsar Wind Nebulae from X-rays to VHE gamma-rays
classification
🌌 astro-ph.HE
keywords
nebulaepulsarpwnesourceswindassociationsbeenextended
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.