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

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

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..381..241t&link_type=abstract

The Second Annual Spitzer Science Center Conference: Infrared Diagnostics of Galaxy Evolution. ASP Conference Series, Vol. 381,

Astronomy and Astrophysics

Astronomy

Scientific paper

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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