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Paper: |
Bulge Formation by the Coalescence of Giant Clumps in Primordial Disk Galaxies |
Volume: |
419, Galaxy Evolution: Emerging Insights and Future Challenges |
Page: |
23 |
Authors: |
Elmegreen, B. G. |
Abstract: |
The observations and evolution of clumpy, high-redshift galaxies are reviewed. Models suggest that the clumps form by gravitational instabilities in a gas-rich disk, interact with each other gravitationally, and then merge in the center where they form a bulge. The model requires smooth gas accretion during galaxy growth. |
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