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Substructure in Dwarf Galaxies

Coleman, Matthew


Recent years have seen a series of large-scale photometric surveys with the aim of detecting substructure in nearby dwarf galaxies. Some of these objects display a varying distribution of each stellar population, reflecting their star formation histories. Also, dwarf galaxies are dominated by dark matter, therefore luminous substructure may represent a perturbation in the underlying dark material. Substructure can also be the effect of tidal interaction, such as the disruption of the...[Show more]

CollectionsANU Research Publications
Date published: 2004
Type: Journal article
Source: Publications of the Astronomical Society of Australia
DOI: 10.1016/j.optcom.2004.03.051


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