The GeV γ-Ray Emission from the Pulsar Wind Nebula DA 495
We present an analysis of GeV γ -ray emission from the region of the pulsar wind nebula (PWN) DA 495, using 17 yr of PASS 8 data from the Fermi Large Area Telescope. In this region, we identify two point sources with markedly different spectra in the GeV band: one exhibits a soft γ -ray spectrum wit...
Gorde:
| Egile Nagusiak: | , |
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| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
IOP Publishing
2026-01-01
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| Saila: | The Astrophysical Journal |
| Gaiak: | |
| Sarrera elektronikoa: | https://doi.org/10.3847/1538-4357/ae3722 |
| Etiketak: |
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