M. Nagashima
The metal enrichment of elliptical galaxies in hierarchical galaxy formation models
Nagashima, M.; Lacey, C.G.; Okamoto, T.; Baugh, C.M.; Frenk, C.S.; Cole, S.
Authors
Professor Cedric Lacey cedric.lacey@durham.ac.uk
Emeritus Professor
T. Okamoto
Professor Carlton Baugh c.m.baugh@durham.ac.uk
Professor
C.S. Frenk
Professor Shaun Cole shaun.cole@durham.ac.uk
Director of the Institute for Computational Cosmology
Abstract
We investigate the metal enrichment of elliptical galaxies in the framework of hierarchical models of galaxy formation. The semi-analytical model we use, which has been used to study the metal enrichment of the intracluster medium (ICM) by Nagashima et al., includes the effects of flows of gas and metals both into and out of galaxies and the processes of metal enrichment due to both type Ia and type II supernovae. We adopt a solar neighbourhood initial mass function (IMF) for star formation in discs, but consider models in which starbursts have either a solar neighbourhood IMF or a top-heavy IMF. We find that the α-element abundance in ellipticals is consistent with observed values only if the top-heavy IMF is used. This result is consistent with our previous study on the metal enrichment of the ICM. We also discuss the abundance ratio of α elements to iron as a function of velocity dispersion and metallicity. We find that models with a top-heavy IMF match the α/Fe ratios observed in typical L* ellipticals, but none of the models reproduces the observed increase of α/Fe with velocity dispersion.
Citation
Nagashima, M., Lacey, C., Okamoto, T., Baugh, C., Frenk, C., & Cole, S. (2005). The metal enrichment of elliptical galaxies in hierarchical galaxy formation models. Monthly Notices of the Royal Astronomical Society: Letters, 363(1), L31-L35. https://doi.org/10.1111/j.1745-3933.2005.00078.x
Journal Article Type | Article |
---|---|
Publication Date | Oct 1, 2005 |
Deposit Date | Feb 20, 2015 |
Publicly Available Date | Feb 20, 2015 |
Journal | Monthly Notices of the Royal Astronomical Society: Letters |
Electronic ISSN | 1745-3933 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 363 |
Issue | 1 |
Pages | L31-L35 |
DOI | https://doi.org/10.1111/j.1745-3933.2005.00078.x |
Keywords | Stars: luminosity function, mass function, Galaxies: clusters: general, Galaxies: formation, Large-scale structure of Universe. |
Public URL | https://durham-repository.worktribe.com/output/1583810 |
Files
Published Journal Article
(147 Kb)
PDF
Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society: Letters ©: 2005 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
You might also like
Towards an accurate model of small-scale redshift-space distortions in modified gravity
(2022)
Journal Article
Fast full N-body simulations of generic modified gravity: derivative coupling models
(2022)
Journal Article
Halo merger tree comparison: impact on galaxy formation models
(2021)
Journal Article
Modelling emission lines in star-forming galaxies
(2021)
Journal Article
Downloadable Citations
About Durham Research Online (DRO)
Administrator e-mail: dro.admin@durham.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2025
Advanced Search