| Issue |
EPJ Web Conf.
Volume 260, 2022
The 16th International Symposium on Nuclei in the Cosmos (NIC-XVI)
|
|
|---|---|---|
| Article Number | 11050 | |
| Number of page(s) | 4 | |
| Section | Poster | |
| DOI | https://doi.org/10.1051/epjconf/202226011050 | |
| Published online | 24 February 2022 | |
https://doi.org/10.1051/epjconf/202226011050
Cosmic Ray production in SNRs of Pulsar Wind Nebulae type at different ages
P.N. Lebedev Physical Institute, Moscow, Russia
* e-mail: sinits@sci.lebedev.ru
Published online: 24 February 2022
The overall observations of plerions from radio to the very high energy gamma-rays could provide information about the evolution of PWN from the young Crab-like to the older stages. The extended MeV-TeV emission from Geminga middle-aged pulsar of ~ 3.4 × 105 year age in SHALON, Milagro, HAWC observations, and Fermi-LAT detection could arise from the PWN associated with the Geminga SNR. The TeV γ-ray emission from 3C 58 PWN whose estimated age varies from ~ 800 to (5 − 7) × 103 years was first detected in year 2011 by SHALON. The overall spectral energy distribution and information about the extension of PWN from radio to GeV-TeV energies from Fermi-LAT and SHALON observations can contribute to particle transport models and also to the understanding of the mechanisms of PWN expanding, which is, in turn, can shed light on the age of 3C 58 and the history of progenitor SN explosion.
© The Authors, published by EDP Sciences, 2022
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