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| Paper: |
A Dust Emission Model for Very Young Galaxies: Expected Properties and Far Infrared Diagnostics |
| Volume: |
381, The Second Annual Spitzer Science Center Conference: Infrared Diagnostics of Galaxy Evolution |
| Page: |
241 |
| Authors: |
Takeuchi, T.T. |
| Abstract: |
Dust plays crucial roles in galaxy formation and evolution. In the early epoch of galaxy evolution dust is only supplied by supernovae (SNe). With the aid of a new physical model of dust production by SNe, we constructed a model of dust emission from forming galaxies. We show the evolution of the spectral energy distribution (SED). Then we adopt this model to a local starbursting dwarf galaxy SBS 0335−052. Further we discuss the SEDs of high redshift galaxies, and consider their observational feasibility. |
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