The diverse evolutionary paths of simulated high-
Massive quiescent galaxies have much smaller physical sizes at high redshift than today. The strong evolution of galaxy size may be caused by progenitor bias, major and minor mergers, adiabatic expansion, and/or renewed star formation, but it is difficult to test these theories observationally. Here...
| Main Authors: | , , , , , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
Oxford University Press,
2017-05-01T13:49:12Z.
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| Subjects: | |
| Online Access: | Get fulltext |