Dusty plasma in active galactic nuclei
نویسندگان
چکیده
Since many years we know that dust in the form of dusty-molecular torus is responsible for obscuration active galactic nuclei (AGN) at large viewing angles and thus classification AGN. Recently, gained some observational theoretical insight into geometry region role dynamics outflow failed winds. We will briefly touch on all these aspects, including our dust-based model (FRADO - Failed Radiatively Accelerated Dusty Outflow) formation Balmer lines
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ژورنال
عنوان ژورنال: European Physical Journal D
سال: 2023
ISSN: ['1434-6060', '1434-6079']
DOI: https://doi.org/10.1140/epjd/s10053-023-00630-8