The Nature of γ-Ray Emission from HESS J1912+101
Since the discovery of HESS J1912+101 at teraelectronvolt energies, its nature has been extensively studied. Due to the absence of X-ray and radio counterparts, whether its γ -ray emission is produced by relativistic electrons or ions is still a matter of debate. We reanalyze its megaelectronvolt to...
Wedi'i Gadw mewn:
| Prif Awduron: | , , |
|---|---|
| Fformat: | Artigo |
| Iaith: | Inglês |
| Cyhoeddwyd: |
IOP Publishing
2023-01-01
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| Cyfres: | The Astrophysical Journal |
| Pynciau: | |
| Mynediad Ar-lein: | https://doi.org/10.3847/1538-4357/ace344 |
| Tagiau: |
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