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The evolution of dust obscuration in galaxies

Dust in galaxies is ubiquitous. It arises from the end stages of stellar evolution, with heavy elements formed over a star's lifetime being distributed throughout a parent galaxy as the star goes supernova.There are numerous approaches to measuring dust obscuration in galaxies. These approaches show a broad trend toward heavier obscuration in galaxies that support higher levels of star formation. However, there is relatively little understanding for why this relationship exists.By analysing the properties of galaxies in the Galaxy And …

Study level
PhD, Master of Philosophy
Faculty
974872
School
School of Chemistry and Physics
Research centre(s)

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