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...
| 出版年: | The Astrophysical Journal |
|---|---|
| 主要な著者: | , , |
| フォーマット: | 論文 |
| 言語: | 英語 |
| 出版事項: |
IOP Publishing
2023-01-01
|
| 主題: | |
| オンライン･アクセス: | https://doi.org/10.3847/1538-4357/ace344 |