Constraints on the Galactic Population of TEV Pulsar Wind Nebulae Using Fermi Large Area Telescope Observations
Langue
en
Article de revue
Ce document a été publié dans
The Astrophysical Journal. 2013, vol. 773, p. 77
American Astronomical Society
Résumé en anglais
Pulsar wind nebulae (PWNe) have been established as the most populous class of TeV gamma-ray emitters. Since launch, the Fermi Large Area Telescope (LAT)identified five high-energy (100MeV