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ISM in nearby elliptical galaxies revealed by AKARI and Spitzer

Published online by Cambridge University Press:  04 October 2008

C. Kramer ,
S. Aalto ,
R. Simon ,
H. Kaneda ,
T. Suzuki ,
K. Haze ,
Y. Okada ,
T. Onaka  and
I. Sakon
H. Kaneda*
Affiliation:
Institute of Space and Astronautical Science, JAXA, Japan
T. Suzuki
Affiliation:
Institute of Space and Astronautical Science, JAXA, Japan
K. Haze
Affiliation:
Institute of Space and Astronautical Science, JAXA, Japan
Y. Okada
Affiliation:
Institute of Space and Astronautical Science, JAXA, Japan
T. Onaka
Affiliation:
Department of Astronomy, Graduate School of Science, University of Tokyo, Japan
I. Sakon
Affiliation:
Department of Astronomy, Graduate School of Science, University of Tokyo, Japan
*
kaneda@ir.isas.jaxa.jp
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Abstract

We performed mid- to far-IR observations of 20 nearby dusty elliptical galaxies with AKARI and Spitzer. We have detected PAHs and extended dust emission from many of our sample galaxies.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 31: Far-Infrared Workshop 2007 , 2008 , pp. 181 - 182
Copyright
© EAS, EDP Sciences, 2008

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References

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