Local Group Analogues
The abundance of satellite galaxies is a critical small-scale test of the standard cosmological model. From comparing the predictions of structure formation in simulations with observations of Local Group dwarf galaxies there is a clear mismatch in the abundance, leading to the so-called “missing sa...
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| Language: | en |
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2012
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| Online Access: | http://hdl.handle.net/10012/7063 |