Dusty plasma in active galactic nuclei

Varování

Publikace nespadá pod Filozofickou fakultu, ale pod Přírodovědeckou fakultu. Oficiální stránka publikace je na webu muni.cz.

Autoři	CZERNY Bozena ZAJAČEK Michal NADDAF Mohammad-Hassan SNIEGOWSKA Marzena PANDA Swayamtrupta ROZANSKA Agata ADHIKARI Tek P. PANDEY Ashwani JAISWAL Vikram Kumar KARAS Vladimír BORKAR Abhijeet MARTÍNEZ-ALDAMA Mary Loli PRINCE Raj
Rok publikování	2023
Druh	Článek v odborném periodiku
Časopis / Zdroj	The European Physical Journal D
Fakulta / Pracoviště MU	Přírodovědecká fakulta
Citace
www	https://doi.org/10.1140/epjd/s10053-023-00630-8
Doi	http://dx.doi.org/10.1140/epjd/s10053-023-00630-8
Klíčová slova	galaxies: active; quasars: emission lines; supermassive black holes; radiative transfer
Popis	For many years we have known that dust in the form of a dusty-molecular torus is responsible for the obscuration in active galactic nuclei (AGN) at large viewing angles and, thus, for the widely used phenomenological classification of AGN. Recently, we gained new observational and theoretical insights into the geometry of the torus region and the role of dust in the dynamics of emerging outflows and failed winds. We will briefly touch on all these aspects and provide a more detailed update of our dust-based model (FRADO—Failed Radiatively Accelerated Dusty Outflow) capable of explaining the processes of formation of Balmer lines in AGN.
Související projekty:	Exploring the Hot Universe and Understanding Comic Feedback