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Infrared observations of AGN
Published online by Cambridge University Press: 01 December 2004
Abstract
We present results from an imaging and spectroscopic study of the dust properties of Seyfert galaxies in the 1-10 μm range. The data are compared to state of the art models of torus emission to constrain geometrical and physical properties of the obscuring medium.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html
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- POSTERS
- Information
- Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS222 , March 2004 , pp. 331 - 332
- Copyright
- © 2004 International Astronomical Union