The origin, nature and distribution of dark matter in the universe form some of the biggest questions in modern astrophysics. Dark matter is distributed on a wide range of scales in the universe. This thesis concentrates on galactic scales, attempting to lower the veil and probe the structure of dark matter in galaxies. (For complete abstract open document)
| Identifer | oai:union.ndltd.org:ADTP/245482 |
| Creators | Trott, Cathryn Margaret |
| Source Sets | Australiasian Digital Theses Program |
| Language | English |
| Detected Language | English |
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