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...
Tallennettuna:
| Päätekijät: | , |
|---|---|
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
IOP Publishing
2026-01-01
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| Sarja: | The Astrophysical Journal |
| Aiheet: | |
| Linkit: | https://doi.org/10.3847/1538-4357/ae3722 |
| Tagit: |
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