The coronal line region of active galactic nuclei
Forbidden coronal lines has traditionally called the attention due to the high-energy photons required for their production (IP >100 eV, where IP is the ionisation potential of the transitions that originate the line). As such, they are regarded as the most highly ionised component of Active Gala...
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| Principais autores: | , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Frontiers Media S.A.
2025-02-01
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| coleção: | Frontiers in Astronomy and Space Sciences |
| Assuntos: | |
| Acesso em linha: | https://www.frontiersin.org/articles/10.3389/fspas.2025.1548632/full |
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