Using Faded Changing-look Quasars to Unveil the Spectral Energy Distribution Evolution of Low-luminosity Active Galactic Nuclei
The structure of accretion flows in low-luminosity active galactic nuclei (AGNs) at low Eddington ratios (∼10 ^−2 –10 ^−3 ) are poorly understood, and can be probed using the spectral energy distributions (SEDs) of faded changing-look (CL) quasars. Previous results using single-epoch X-ray and rest-...
Guardado en:
| Autores principales: | , , , , , , , , , |
|---|---|
| Formato: | Artigo |
| Lenguaje: | Inglês |
| Publicado: |
IOP Publishing
2026-01-01
|
| Colección: | The Astrophysical Journal |
| Materias: | |
| Acceso en línea: | https://doi.org/10.3847/1538-4357/ae5191 |
| Etiquetas: |
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
