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...
Na minha lista:
| Principais autores: | , , , , , |
|---|---|
| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
IOP Publishing
2026-01-01
|
| Serier: | The Astrophysical Journal |
| Fag: | |
| Online adgang: | https://doi.org/10.3847/1538-4357/ae3d06 |
| Tags: |
Ingen Tags, Vær først til at tagge denne postø!
|