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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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