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Model for Infrared Properties of Extremely Young Galaxies

  • T. T. Takeuchi (a1), H. Hirashita (a2), T. T. Ishii (a3), L. K. Hunt (a4) and A. Ferrara (a5)...

Abstract

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.

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Copyright

References

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

Model for Infrared Properties of Extremely Young Galaxies

  • T. T. Takeuchi (a1), H. Hirashita (a2), T. T. Ishii (a3), L. K. Hunt (a4) and A. Ferrara (a5)...

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