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The impact of ISM turbulence, clustered star formation and feedback on galaxy mass assembly through cold flows and mergers

Abstract:

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. Indeed there is still much to understand about the detailed physics of each process in isolation. While these formation channels have been studied using hydrodynamical simulations, here we study their ...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1017/S1743921311022848

Authors


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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
Publisher:
Cambridge University Press
Journal:
Proceedings of the International Astronomical Union More from this journal
Volume:
6
Issue:
S277
Pages:
234-237
Publication date:
2011-12-05
DOI:
EISSN:
1743-9221
ISSN:
1743-9213
Keywords:
Pubs id:
pubs:205754
UUID:
uuid:2291dbb2-eb56-4929-b154-b3a5968f2ab4
Local pid:
pubs:205754
Source identifiers:
205754
Deposit date:
2012-12-19

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