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Infrared observations of AGN

Published online by Cambridge University Press:  01 December 2004

P. Lira ,
F. Marín ,
L. Videla ,
A. Alonso-Herrero ,
D. M. Alexander  and
M. Ward
P. Lira
Affiliation:
Universidad de Chile, Casilla 36-D, Santiago, Chile
F. Marín
Affiliation:
Universidad de Chile, Casilla 36-D, Santiago, Chile
L. Videla
Affiliation:
Universidad de Chile, Casilla 36-D, Santiago, Chile
A. Alonso-Herrero
Affiliation:
DAMIR-IEM, C. Serrano 113-121, 28006 Madrid, Spain
D. M. Alexander
Affiliation:
Cambridge University, Madingley Road, Cambridge CB3 0HA, UK
M. Ward
Affiliation:
Leicester University, Leicester LE1 7RH, UK
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Abstract

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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

Type
POSTERS
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS222 , March 2004 , pp. 331 - 332
Copyright
© 2004 International Astronomical Union