High-energy Pulsar Wind Nebulae and SuperNova Remnants

Giordano, F. (2011) High-energy Pulsar Wind Nebulae and SuperNova Remnants. Il nuovo cimento C, 34 (3). pp. 183-189. ISSN 1826-9885

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After the second year of Fermi orbiting, the number of galactic sources associated with Pulsar Wind Nebulae (PWNe) and SuperNova Remnants (SNRs) has largely increased. For all these sources multi-wavelenghts spectral energy distributions have been investigated and information about acceleration mechanisms and interaction sites have been collected and studied. The GeV-TeV connection of some recently detected sources will be presented and different interpretation of the observed spectra will be discussed.

Item Type: Article
Uncontrolled Keywords: γ-ray ; Origin, formation, evolution, age, and star formation ; Supernova remnants ; Cosmic rays (including sources, origin, acceleration, and interactions)
Subjects: 500 Scienze naturali e Matematica > 530 Fisica
Depositing User: Marina Spanti
Date Deposited: 06 Apr 2020 18:35
Last Modified: 06 Apr 2020 18:35
URI: http://eprints.bice.rm.cnr.it/id/eprint/17265

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