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The origin of the radio emission in active galactic nuclei (AGN) is still debated. Multiple physical mechanisms can contribute to the spectrum at these frequencies, including relativistic jets, the jet base, outflows, star formation, and synchrotron emission from the hot corona. Recently, new extrem...
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| Autors principals: | , , , , , , , , , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
EDP Sciences
2026-04-01
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| Col·lecció: | Astronomy & Astrophysics |
| Matèries: | |
| Accés en línia: | https://www.aanda.org/articles/aa/full_html/2026/04/aa58552-25/aa58552-25.html |
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