Pulsar Wind Nebulae from X-rays to VHE gamma-rays
Oleg Kargaltsev, George G. Pavlov, and Martin Durant
TL;DR
This paper reviews recent advances in X-ray and TeV observations of pulsar wind nebulae, highlighting their properties and the increasing number of associations with extended VHE gamma-ray sources.
Contribution
It provides a comprehensive overview of recent observational progress and summarizes key properties of PWNe from X-ray to VHE gamma-ray data.
Findings
Growing number of associations between VHE sources and PWNe
Enhanced understanding of PWN properties across wavelengths
Progress in observational techniques and data analysis
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.
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Astrophysics and Cosmic Phenomena · Gamma-ray bursts and supernovae