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...
I tiakina i:
| Ngā kaituhi matua: | , , |
|---|---|
| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
IOP Publishing
2023-01-01
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| Rangatū: | The Astrophysical Journal |
| Ngā marau: | |
| Urunga tuihono: | https://doi.org/10.3847/1538-4357/ace344 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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