Radiatively enhanced elasticity and turbulence in clumpy tori of Active Galactic Nuclei
Cosmology and Nongalactic Astrophysics
2010-07-02 v3
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.
Cite
@article{arxiv.0911.4971,
title = {Radiatively enhanced elasticity and turbulence in clumpy tori of Active Galactic Nuclei},
author = {Martin Krause and Marc Schartmann and Andreas Burkert and Max Camenzind},
journal= {arXiv preprint arXiv:0911.4971},
year = {2010}
}
Comments
10 pages, 5 figures, accepted by MNRAS, this paper has been withdrawn by the authors due to an essential flaw in the assumptions