Angular momentum transfer to a Milky Way disk at high redshift
An Adaptive Mesh Refinement cosmological resimulation is analyzed in order to test whether filamentary flows of cold gas are responsible for the build-up of angular momentum within a Milky Way like disk at z>=3. A set of algorithms is presented that takes advantage of the high spatial resolut...
| 主要な著者: | , , , , |
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| フォーマット: | Journal article |
| 出版事項: |
2015
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