The impact of accurate distances to dwarf elliptical galaxies on cosmology
The Surface Brightness Fluctuation method has been shown to be a powerful distance indicator for dwarf elliptical galaxies to very low surface brightness levels. It is applicable to stellar systems that are out of reach for classical indicators requiring
|Collections||ANU Research Publications|
|Book Title:||Near-field Cosmology with Dwarf Elliptical Galaxies|
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