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arXiv · 2211.11022

Dusty plasma in active galactic nuclei

Bożena Czerny·Michal Zajaček·Mohammad-Hassan Naddaf·Marzena Sniegowska·Swayamtrupta Panda·Agata Różanska·Tek P. Adhikari·Ashwani Pandey·Vikram Kumar Jaiswal·Vladimír Karas·Abhijeet Borkar·Mary Loli Martínez-Aldama·Raj Prince
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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.

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Bożena Czerny, Michal Zajaček, Mohammad-Hassan Naddaf, Marzena Sniegowska, Swayamtrupta Panda, Agata Różanska, Tek P. Adhikari, Ashwani Pandey, Vikram Kumar Jaiswal, Vladimír Karas, Abhijeet Borkar, Mary Loli Martínez-Aldama, Raj Prince. 2022-11-20. Dusty plasma in active galactic nuclei. https://doi.org/10.1140/epjd%2Fs10053-023-00630-8

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