Evolving Starburst Model of FIR/sub-mm/mm Line Emission and Its Applications to M82 and Nearby Luminous Infrared Galaxies
This thesis presents a starburst model for far-infrared/sub-millimeter/millimeter (FIR/sub-mm/mm) line emission of molecular and atomic gas in an evolving starburst region, which is treated as an ensemble of non-interacting hot bubbles which drive spherical shells of swept-up gas into a surrounding...
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Language: | en_ca |
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2009
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Online Access: | http://hdl.handle.net/1807/26484 |