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A variety of torus models for the infrared emission of AGN has become available in literature over the last decade. This includes radiative transfer models using smooth or clumpy dust and hydrodynamic models. I will review the various types of models that are currently in use and point out their main similarities, differences, and limits when it comes to interpreting observations. Finally, current and future observational challenges for these models are discussed.

生成讲解博客的中文版本

生成AI智能校验的中文版本