Ultra-thick warm absorbers: Enlarging the parameter space of AGN ionised outflows

Context. The analysis of X-ray absorption features in active galactic nuclei (AGN) provides a wealth of information about the physical properties of the matter surrounding supermassive black holes (SMBHs). While standard correlations between the ionisation state, column density, and velocity typical...

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Detalles Bibliográficos

Principais autores:	Middei R., Piconcelli E., Nardini E., Marinucci A., Laurenti M., Luminari A., Trindade Falcão A., Tortosa A., Perri M., Puccetti S., Król D. Ł., Borrelli L.
Formato:	Artigo
Idioma:	Inglês
Publicado:	EDP Sciences 2026-06-01
Series:	Astronomy & Astrophysics
Assuntos:	galaxies: active galaxies: nuclei
Acceso en liña:	https://www.aanda.org/articles/aa/full_html/2026/06/aa59321-26/aa59321-26.html
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