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Model for Infrared Properties of Extremely Young Galaxies

Published online by Cambridge University Press:  26 May 2016

T. T. Takeuchi ,
H. Hirashita ,
T. T. Ishii ,
L. K. Hunt  and
A. Ferrara
T. T. Takeuchi
Affiliation:
NAOJ, Tokyo, Japan
H. Hirashita
Affiliation:
Nagoya U., Nagoya, Japan
T. T. Ishii
Affiliation:
Kyoto U., Kyoto, Japan
L. K. Hunt
Affiliation:
CAISMI-IRA/CNR, Firenze, Italy
A. Ferrara
Affiliation:
SISSA, Trieste, Italy

Abstract

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We constructed a model of the infrared spectral energy distribution for very young galaxies by taking into account the dust size distribution in the early stage of galaxy evolution.

Type
Part 2. Origin
Information
Symposium - International Astronomical Union , Volume 217: Recycling Intergalactic and Interslettar Matter , 2004 , pp. 214 - 215
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Hirashita, H., Hunt, L. K., & Ferrara, A. 2002, MNRAS, 330, L19.CrossRefGoogle Scholar
Takeuchi, T. T., Hirashita, H., Ishii, T. T., Hunt, L. K., & Ferrara, A. 2003, MNRAS, 343, 839.CrossRefGoogle Scholar
Todini, P., & Ferrara, A. 2001, MNRAS, 325, 726.CrossRefGoogle Scholar