Since many years we know that dust in the form of the dusty-molecular torus
is responsible for the obscuration in active galactic nuclei (AGN) at large
viewing angles and thus for the classification of AGN. Recently, we gained some
observational and theoretical insight into geometry of the region and the role
of the dust in the dynamics of the outflow and failed winds. We will briefly
touch on all these aspects, including our dust-based model (FRADO - Failed
Radiatively Accelerated Dusty Outflow) of the formation of the Balmer lines in
AGN.
cite arxiv:2211.11022Comment: Partially based on talk at 31st Symposium on the Physics of Ionized Gases in Belgrade, submitted to the European Physical Journal D Topical Issue: "Physics of Ionized Gases and Spectroscopy of Isolated Complex Systems: Fundamentals and Applications"
%0 Generic
%1 czerny2022dusty
%A Czerny, Bożena
%A Zajaček, Michal
%A Naddaf, Mohammad-Hassan
%A Sniegowska, Marzena
%A Panda, Swayamtrupta
%A Różanska, Agata
%A Adhikari, Tek P.
%A Pandey, Ashwani
%A Jaiswal, Vikram Kumar
%A Karas, Vladimír
%A Borkar, Abhijeet
%A Martínez-Aldama, Mary Loli
%A Prince, Raj
%D 2022
%K library
%T Dusty plasma in active galactic nuclei
%U http://arxiv.org/abs/2211.11022
%X Since many years we know that dust in the form of the dusty-molecular torus
is responsible for the obscuration in active galactic nuclei (AGN) at large
viewing angles and thus for the classification of AGN. Recently, we gained some
observational and theoretical insight into geometry of the region and the role
of the dust in the dynamics of the outflow and failed winds. We will briefly
touch on all these aspects, including our dust-based model (FRADO - Failed
Radiatively Accelerated Dusty Outflow) of the formation of the Balmer lines in
AGN.
@misc{czerny2022dusty,
abstract = {Since many years we know that dust in the form of the dusty-molecular torus
is responsible for the obscuration in active galactic nuclei (AGN) at large
viewing angles and thus for the classification of AGN. Recently, we gained some
observational and theoretical insight into geometry of the region and the role
of the dust in the dynamics of the outflow and failed winds. We will briefly
touch on all these aspects, including our dust-based model (FRADO - Failed
Radiatively Accelerated Dusty Outflow) of the formation of the Balmer lines in
AGN.},
added-at = {2022-11-22T09:00:10.000+0100},
author = {Czerny, Bożena and Zajaček, Michal and Naddaf, Mohammad-Hassan and Sniegowska, Marzena and Panda, Swayamtrupta and Różanska, Agata and Adhikari, Tek P. and Pandey, Ashwani and Jaiswal, Vikram Kumar and Karas, Vladimír and Borkar, Abhijeet and Martínez-Aldama, Mary Loli and Prince, Raj},
biburl = {https://www.bibsonomy.org/bibtex/2b01e52b3cd89680f5caedb7f311fdc2c/gpkulkarni},
description = {Dusty plasma in active galactic nuclei},
interhash = {6d6a810904538f132a3934906c66d7e5},
intrahash = {b01e52b3cd89680f5caedb7f311fdc2c},
keywords = {library},
note = {cite arxiv:2211.11022Comment: Partially based on talk at 31st Symposium on the Physics of Ionized Gases in Belgrade, submitted to the European Physical Journal D Topical Issue: "Physics of Ionized Gases and Spectroscopy of Isolated Complex Systems: Fundamentals and Applications"},
timestamp = {2022-11-22T09:00:10.000+0100},
title = {Dusty plasma in active galactic nuclei},
url = {http://arxiv.org/abs/2211.11022},
year = 2022
}