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Model for Infrared Properties of Extremely Young Galaxies
Published online by Cambridge University Press: 26 May 2016
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
Takeuchi, T. T., Hirashita, H., Ishii, T. T., Hunt, L. K., & Ferrara, A.
2003, MNRAS, 343, 839.CrossRefGoogle Scholar
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