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Mid- and Far-Infrared Study of X-ray-emitting Dusty Elliptical Galaxies

Published online by Cambridge University Press:  01 August 2006

H. Kaneda ,
T. Onaka ,
T. Kitayama ,
Y. Okada  and
I. Sakon
H. Kaneda
Affiliation:
Institute of Space and Astronautical Science, Sagamihara, Kanagawa 229-8510, Japan email: kaneda@ir.isas.jaxa.jp
T. Onaka
Affiliation:
Department of Astronomy, University of Tokyo, Bunkyo-ku, Tokyo 113-0003, Japan
T. Kitayama
Affiliation:
Department of Physics, Toho University, Funabashi, Chiba 274-8510, Japan
Y. Okada
Affiliation:
Institute of Space and Astronautical Science, Sagamihara, Kanagawa 229-8510, Japan email: kaneda@ir.isas.jaxa.jp
I. Sakon
Affiliation:
Department of Astronomy, University of Tokyo, Bunkyo-ku, Tokyo 113-0003, Japan
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Abstract

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We study nearby X-ray-emitting dusty elliptical galaxies in mid- and far-infrared by using the Spitzer Space Telescope and AKARI, the Japanese infrared astronomical satellite.

Keywords

ISM: dustextinction — galaxies: elliptical and lenticularcD — galaxies: ISM
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 211
Copyright
Copyright © International Astronomical Union 2007

References

Kaneda, H., Onaka, T., & Sakon, I. 2005, ApJ, 632, L83.CrossRefGoogle Scholar