The impact of ISM turbulence, clustered star formation and feedback on galaxy mass assembly through cold flows and mergers
<p>Two of the dominant channels for galaxy mass assembly are cold flows (cold gas supplied via the filaments of the cosmic web) and mergers. How these processes combine in a cosmological setting, at both low and high redshift, to produce the whole zoo of galaxies we observe is largely unknown...
| Những tác giả chính: | , , , , , |
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| Định dạng: | Journal article |
| Được phát hành: |
Cambridge University Press
2011
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