M. Sharma
The chemical imprint of the bursty nature of Milky Way's progenitors
Sharma, M.; Theuns, T.; Frenk, C.
Authors
Professor Tom Theuns tom.theuns@durham.ac.uk
Professor
Professor Carlos Frenk c.s.frenk@durham.ac.uk
Professor
Abstract
Carbon-enhanced metal-poor (CEMP) stars with low abundances of neutron capture elements (CEMP-no stars) are ubiquitous among metal-poor stars in the Milky Way. Recent observations have uncovered their two subgroups that differ in the carbon to magnesium ([C/Mg]) abundance ratio. Here, we demonstrate that similar abundance patterns are also present in Milky Way-like galaxies in the EAGLE cosmological hydrodynamical simulation, where these patterns originate from the fact that stars may form from gas enriched predominantly by asymptotic giant branch (AGB) stars or by type II supernovae. This occurs when stars form in the poorly mixed interstellar medium of Milky Way progenitor galaxies that are undergoing bursty star formation. The CEMP-no stars with lower [C/Mg] form at the onset of a starburst from gas enriched by low-metallicity type II supernovae that power a strong outflow, quenching further star formation. When star formation resumes following cosmological gas accretion, the CEMP-no stars with higher [C/Mg] form, with enrichment by AGB ejecta evident in their higher abundance of barium and lower abundance of magnesium. This suggests that bursty star formation in the progenitors of the Galaxy leaves a permanent imprint in the abundance patterns of CEMP stars.
Citation
Sharma, M., Theuns, T., & Frenk, C. (2019). The chemical imprint of the bursty nature of Milky Way's progenitors. Monthly Notices of the Royal Astronomical Society, 482(1), L145-L149. https://doi.org/10.1093/mnrasl/sly195
Journal Article Type | Article |
---|---|
Acceptance Date | Oct 9, 2018 |
Online Publication Date | Oct 17, 2018 |
Publication Date | Jan 1, 2019 |
Deposit Date | Nov 21, 2018 |
Publicly Available Date | Nov 21, 2018 |
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 | 482 |
Issue | 1 |
Pages | L145-L149 |
DOI | https://doi.org/10.1093/mnrasl/sly195 |
Public URL | https://durham-repository.worktribe.com/output/1313276 |
Files
Published Journal Article
(2 Mb)
PDF
Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2018 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
You might also like
The impact and response of mini-haloes and the interhalo medium on cosmic reionization
(2024)
Journal Article
The FLAMINGO project: revisiting the S8 tension and the role of baryonic physics
(2023)
Journal Article
Where shadows lie: reconstruction of anisotropies in the neutrino sky
(2023)
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