A GROWTH-RATE INDICATOR FOR COMPTON-THICK ACTIVE GALACTIC NUCLEI

Due to their heavily obscured central engines, the growth rate of Compton-thick (CT) active galactic nuclei (AGNs) is difficult to measure. A statistically significant correlation between the Eddington ratio, lambda(Edd), and the X-ray power-law index, Gamma, observed in unobscured AGNs offers an es...

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Detalles Bibliográficos
Autores principales: Brightman, M., Masini, A., Ballantyne, D. R., Balokovic, M., Brandt, W. N., Chen, C. -T., Comastri, A., Farrah, D., Gandhi, P., Harrison, F. A., Ricci, C., Stern, D., Walton, D. J.
Formato: Artículo (Article)
Idioma:Inglés (English)
Publicado: 2025
Materias:
black hole physics
galaxies: general
galaxies: nuclei
galaxies: Seyfert
masers
Acceso en línea:https://repositorio.uc.cl/handle/11534/101436

Internet

https://repositorio.uc.cl/handle/11534/101436

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