- Abstract:
-
Observations and theoretical simulations have established a framework for galaxy formation and evolution in the young Universe. Galaxies formed as baryonic gas cooled at the centres of collapsing dark-matter haloes; mergers of haloes and galaxies then led to the hierarchical build-up of galaxy mass. It remains unclear, however, over what timescales galaxies were assembled and when and how bulges and disks - the primary components of present-day galaxies - were formed. It is also puzzling that...
Expand abstract - Publisher copy:
- 10.1038/nature05052
-
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- Journal:
- Nature
- Volume:
- 442
- Issue:
- 7104
- Pages:
- 786-789
- Publication date:
- 2006-08-17
- DOI:
- EISSN:
-
1476-4679
- ISSN:
-
0028-0836
- URN:
-
uuid:0c99545f-c303-436c-820e-f89f6f792ab5
- Source identifiers:
-
252232
- Local pid:
- pubs:252232
- Language:
- English
- Copyright date:
- 2006
Journal article
The rapid formation of a large rotating disk galaxy three billion years after the Big Bang
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