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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Abstract
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 |
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| 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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