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The origin and evolution of the mass-metallicity relation using GalICS

Abstract:

The Galaxies in Cosmological Simulations (GalICS) semi-analytical model of hierarchical galaxy formation is used to investigate the effects of different galactic properties, including star formation rate (SFR) and outflows, on the shape of the mass–metallicity relation and to predict the relation for galaxies at redshift z= 2.27 and 3.54. Our version of GalICS has the chemical evolution implemented in great detail and is less heavily reliant on approximations, such as instantaneo...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Version of record

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Publisher copy:
10.1111/j.1365-2966.2010.17593.x

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Institution:
University of Oxford
Department:
Oxford, MPLS, Physics, Astrophysics
Role:
Author
Publisher:
Oxford University Press (OUP) Publisher's website
Journal:
Monthly Notices of the Royal Astronomical Society Journal website
Volume:
410
Issue:
4
Pages:
2203–2216
Publication date:
2011-01-13
Acceptance date:
2010-08-24
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
URN:
uuid:65e0cf98-9c2c-41c9-a53a-eff1081d1526
Source identifiers:
205751
Local pid:
pubs:205751

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