Physically Modeling High-Redshift Ultraluminous Infrared Galaxies
We have used a combination of hydrodynamical simulations, dust radiative transfer, and an empirically based analytical model for galaxy number densities and merger rates in order to physically model the bright high-redshift submillimeter-selected galaxy (SMG) population. We report the results of thr...
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| Language: | en_US |
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Harvard University
2013
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| Online Access: | http://dissertations.umi.com/gsas.harvard:10008 http://nrs.harvard.edu/urn-3:HUL.InstRepos:10121984 |