A Dust Emission Model for Very Young Galaxies: Expected Properties and Far Infrared Diagnostics

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dc.creatorTakeuchi, Tsutomu T.
dc.date2006-03-14
dc.date.accessioned2026-07-07T07:01:04Z
dc.date.available2026-07-07T07:01:04Z
dc.descriptionDust 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.
dc.description8 pages, 4 figures, to appear in the proceedings of "Infrared Diagnostics of Galaxy Evolution"
dc.identifierhttps://arxiv.org/abs/astro-ph/0603337
dc.identifierhttp://arxiv.org/abs/astro-ph/0603337
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/108168
dc.subjectAstrophysics
dc.titleA Dust Emission Model for Very Young Galaxies: Expected Properties and Far Infrared Diagnostics
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