CLOUD DISTRIBUTION IN OBSCURING TORI OF ACTIVE GALACTIC NUCLEI

• Дата: 2015
• Автор: Bannikova, E. Yu.
• Формат: Стаття
• Мова: rus
• Опубліковано: Видавничий дім «Академперіодика» 2015
• Теми: active galactic nuclei; unified scheme; obscuring torus; активные ядра галактик; унифицированная схема; затеняющий тор; активні ядра галактик; уніфікована схема; затінюючий тор
• Онлайн доступ: http://rpra-journal.org.ua/index.php/ra/article/view/1215
• Назва журналу: Radio physics and radio astronomy

In the framework of N-body simulations, we have investigated the influence of initial conditions on the evolution of self-gravitating torus being in the active galactic nuclei (AGN), as well as evolution of distribution of particles (clouds) by their orbital elements analysed. The results of simulations show that stability of a geometrically thick torus in AGN can be explained by the motion of clouds in the torus by inclined and eccentric orbits. The scenario of torus formation being related to the beginning of the AGN’s stage is suggested.Key words: active galactic nuclei, unified scheme, obscuring torusManuscript submitted 28.05.2015Radio phys. radio astron. 2015, 20(3): 191-204REFERENCES1. BIANCHI, S., MAIOLINO, R. and RISALITI, G., 2012. AGN Obscuration and the Unified Model. Adv. Astron., id. 782030. 2. NETZER, H., 2013. The physics and evolution of active galactic nuclei. New York: Cambridge university press. DOI: https://doi.org/10.1017/CBO9781139109291 3. NETZER, H., 2015. 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