M. Furlong
Evolution of galaxy stellar masses and star formation rates in the EAGLE simulations
Furlong, M.; Bower, R.G.; Theuns, T.; Schaye, J.; Crain, R.A.; Schaller, M.; Dalla Vecchia, C.; Frenk, C.S.; McCarthy, I.G.; Helly, J.; Jenkins, A.; Rosas-Guevara, Y.M.
Authors
R.G. Bower
Professor Tom Theuns tom.theuns@durham.ac.uk
Professor
J. Schaye
R.A. Crain
M. Schaller
C. Dalla Vecchia
Professor Carlos Frenk c.s.frenk@durham.ac.uk
Professor
I.G. McCarthy
J. Helly
Professor Adrian Jenkins a.r.jenkins@durham.ac.uk
Professor
Y.M. Rosas-Guevara
Abstract
We investigate the evolution of galaxy masses and star formation rates in the Evolution and Assembly of Galaxies and their Environment (eagle) simulations. These comprise a suite of hydrodynamical simulations in a Λ cold dark matter cosmogony with subgrid models for radiative cooling, star formation, stellar mass-loss and feedback from stars and accreting black holes. The subgrid feedback was calibrated to reproduce the observed present-day galaxy stellar mass function and galaxy sizes. Here, we demonstrate that the simulations reproduce the observed growth of the stellar mass density to within 20 per cent. The simulations also track the observed evolution of the galaxy stellar mass function out to redshift z = 7, with differences comparable to the plausible uncertainties in the interpretation of the data. Just as with observed galaxies, the specific star formation rates of simulated galaxies are bimodal, with distinct star forming and passive sequences. The specific star formation rates of star-forming galaxies are typically 0.2 to 0.5 dex lower than observed, but the evolution of the rates track the observations closely. The unprecedented level of agreement between simulation and data across cosmic time makes eagle a powerful resource to understand the physical processes that govern galaxy formation.
Citation
Furlong, M., Bower, R., Theuns, T., Schaye, J., Crain, R., Schaller, M., …Rosas-Guevara, Y. (2015). Evolution of galaxy stellar masses and star formation rates in the EAGLE simulations. Monthly Notices of the Royal Astronomical Society, 450(4), 4486-4504. https://doi.org/10.1093/mnras/stv852
Journal Article Type | Article |
---|---|
Acceptance Date | Apr 15, 2015 |
Publication Date | Jul 11, 2015 |
Deposit Date | Feb 10, 2016 |
Publicly Available Date | Feb 16, 2016 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 450 |
Issue | 4 |
Pages | 4486-4504 |
DOI | https://doi.org/10.1093/mnras/stv852 |
Keywords | Galaxies: abundances, Galaxies: evolution, Galaxies: formation, Galaxies: high-redshift, Galaxies: star formation. |
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Copyright Statement
This article has been accepted for publication in Monthly notices of the Royal Astronomical Society ©: 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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