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Dusty Torus Formation by Anisotropic Radiative Pressure Feedback of Active Galactic Nuclei

Dusty Torus Formation by Anisotropic Radiative Pressure Feedback of Active Galactic Nuclei. Shuang-Nan Zhang Institute of High Energy Physics and National Astronomical Observatories of China Chinese Academy of Sciences. Liu,Y. & Zhang, S.N., 2011, ApJL, 728, L44. The unified model of AGN.

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Radio loud bl lac - PowerPoint PPT Presentation

Dusty Torus Formation by Anisotropic Radiative Pressure Feedback of Active Galactic Nuclei