Rotation curve mass modeling of disk galaxies
The standard Cold Dark Matter (CDM) model for cosmological structure formation has been remarkably successful in explaining the observed large scale structure of the universe. At the scale of individual galaxies, however, CDM faces serious challenges; one of these is the apparent discrepancy between...
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| Format: | Others |
| Language: | English |
| Published: |
2009
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| Online Access: | http://hdl.handle.net/2429/14128 |