Properties and Possible Physical Origins of γ-Ray Emission in Extreme Synchrotron Blazars
Extreme synchrotron blazars, characterized by a first peak in their broadband spectral energy distributions (SEDs) at frequencies exceeding 10 ^17 Hz, often exhibit a second peak beyond 1 TeV. These sources serve as ideal laboratories for studying particle acceleration and radiation mechanisms in re...
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| Autors principals: | , , , , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
IOP Publishing
2026-01-01
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| Col·lecció: | The Astrophysical Journal |
| Matèries: | |
| Accés en línia: | https://doi.org/10.3847/1538-4357/ae3d06 |
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