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arXiv · 0911.4971

Radiatively enhanced elasticity and turbulence in clumpy tori of Active Galactic Nuclei

Martin Krause·Marc Schartmann·Andreas Burkert·Max Camenzind
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Abstract

The paper assumes radiation forces proportional to distance between equal temperature clouds. However, we assume there are clouds in any direction. The forces then cancel almost entirely, besides small velocity effects. Therefore, the presented theory is inadequate.

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Martin Krause, Marc Schartmann, Andreas Burkert, Max Camenzind. 2009-11-25. Radiatively enhanced elasticity and turbulence in clumpy tori of Active Galactic Nuclei. https://arxiv.org/abs/0911.4971

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