| Título |
The Ultra-High-Energy Source MGRO J1908+06 |
| Tipo |
Congreso |
| Sub-tipo |
Memoria |
| Descripción |
37th International Cosmic Ray Conference, ICRC 2021 |
| Resumen |
The TeV gamma-ray source MGRO J1908+06 is one of the highest-energy sources known, with observed emission by the High Altitude Water Cherenkov (HAWC) Observatory extending well past 100 TeV. The source exhibits both energy-dependent morphology and a spatially-dependent spectral index. The emission is likely to be dominantly leptonic, and associated with the radio-quiet PSR J1907+0602. However, one-population models do not describe the data well; a second particle population is needed to explain the shape of the spectral energy distribution at the highest energies. This component can be well-described by either leptonic or hadronic hypotheses. We discuss this feature and implications for detection by multi-wavelength and multi-messenger experiments. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0). |
| Observaciones |
Proceedings of Science, v. 395 |
| Lugar |
Virtual, online |
| País |
Indefinido |
| No. de páginas |
Article number 810 |
| Vol. / Cap. |
|
| Inicio |
2021-07-12 |
| Fin |
2021-07-23 |
| ISBN/ISSN |
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