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Nuclear IR SED of Type 2 Seyfert Galaxies

Published online by Cambridge University Press:  03 June 2010

L. Videla ,
P. Lira ,
A. Alonso-Herrero ,
D. M. Alexander  and
M. Ward
L. Videla
Affiliation:
Astronomy Department, University of Chile, Santiago, Chile
P. Lira
Affiliation:
Astronomy Department, University of Chile, Santiago, Chile
A. Alonso-Herrero
Affiliation:
DAMIR, IEM, CSIC, Spain
D. M. Alexander
Affiliation:
Department of Physics, Durham University, Durham, UK
M. Ward
Affiliation:
Department of Physics, Durham University, Durham, UK
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We obtained deep images for 49 Seyfert 2 galaxies in 6 infrared bands: J, H, K, L, M, and N with the VLT at Paranal, the NTT at La Silla, and Gemini at Pachón, to compile their nuclear infrared (IR) spectral energy distributions (SEDs). These galaxies were extracted from the Extended 12 μm Galaxy Sample (Rush et al. 1993).

Keywords

galaxies: Seyfertinfrared: galaxies
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S267: Co-Evolution of Central Black Holes and Galaxies , August 2009 , pp. 145
Copyright
Copyright © International Astronomical Union 2010

References

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