Effects of secular growth and mergers on the evolution of metallicity gradients and azimuthal variations in a Milky Way-like galaxy
(2025) In Astronomy and Astrophysics 694.- Abstract
We analyzed the evolution of the radial profiles and the azimuthal variations of the stellar metallicities from the VINTERGATAN simulation of a Milky Way-like galaxy. We find that negative gradients exist as soon as the disk settles at high redshift, and are maintained throughout the long-term evolution of the galaxy, including during major merger events. The inside-out growth of the disk and an overall outward radial migration tend to flatten these gradients in time. Major merger events only have a moderate and shortlived imprint on the [Fe/H] distributions with almost no radial dependence. The reason lies in the timescale for enrichment in Fe being significantly longer than the duration of the starbursts episodes, themselves slower... (More)
We analyzed the evolution of the radial profiles and the azimuthal variations of the stellar metallicities from the VINTERGATAN simulation of a Milky Way-like galaxy. We find that negative gradients exist as soon as the disk settles at high redshift, and are maintained throughout the long-term evolution of the galaxy, including during major merger events. The inside-out growth of the disk and an overall outward radial migration tend to flatten these gradients in time. Major merger events only have a moderate and shortlived imprint on the [Fe/H] distributions with almost no radial dependence. The reason lies in the timescale for enrichment in Fe being significantly longer than the duration of the starbursts episodes, themselves slower than dynamical mixing during typical interactions. It results in signatures of major mergers becoming undetectable in [Fe/H] only a few megayears after pericenter passages. We note that considering other tracers like the warm interstellar medium, or monitoring the evolution of the metallicity gradient as a single value instead of a radial full profile could lead to different interpretations; we warn against oversimplifying this complex problem.
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- author
- Renaud, Florent LU ; Ratcliffe, Bridget ; Minchev, Ivan ; Haywood, Misha ; Di Matteo, Paola ; Agertz, Oscar LU and Romeo, Alessandro B.
- organization
- publishing date
- 2025-02
- type
- Contribution to journal
- publication status
- published
- subject
- keywords
- Galaxy: disk, Galaxy: evolution, Methods: numerical
- in
- Astronomy and Astrophysics
- volume
- 694
- article number
- A56
- publisher
- EDP Sciences
- external identifiers
-
- scopus:85217012720
- ISSN
- 0004-6361
- DOI
- 10.1051/0004-6361/202452219
- language
- English
- LU publication?
- yes
- id
- b7454284-576f-4f0a-bbb7-d411940db667
- date added to LUP
- 2025-04-07 14:52:57
- date last changed
- 2025-04-07 14:53:47
@article{b7454284-576f-4f0a-bbb7-d411940db667,
abstract = {{<p>We analyzed the evolution of the radial profiles and the azimuthal variations of the stellar metallicities from the VINTERGATAN simulation of a Milky Way-like galaxy. We find that negative gradients exist as soon as the disk settles at high redshift, and are maintained throughout the long-term evolution of the galaxy, including during major merger events. The inside-out growth of the disk and an overall outward radial migration tend to flatten these gradients in time. Major merger events only have a moderate and shortlived imprint on the [Fe/H] distributions with almost no radial dependence. The reason lies in the timescale for enrichment in Fe being significantly longer than the duration of the starbursts episodes, themselves slower than dynamical mixing during typical interactions. It results in signatures of major mergers becoming undetectable in [Fe/H] only a few megayears after pericenter passages. We note that considering other tracers like the warm interstellar medium, or monitoring the evolution of the metallicity gradient as a single value instead of a radial full profile could lead to different interpretations; we warn against oversimplifying this complex problem.</p>}},
author = {{Renaud, Florent and Ratcliffe, Bridget and Minchev, Ivan and Haywood, Misha and Di Matteo, Paola and Agertz, Oscar and Romeo, Alessandro B.}},
issn = {{0004-6361}},
keywords = {{Galaxy: disk; Galaxy: evolution; Methods: numerical}},
language = {{eng}},
publisher = {{EDP Sciences}},
series = {{Astronomy and Astrophysics}},
title = {{Effects of secular growth and mergers on the evolution of metallicity gradients and azimuthal variations in a Milky Way-like galaxy}},
url = {{http://dx.doi.org/10.1051/0004-6361/202452219}},
doi = {{10.1051/0004-6361/202452219}},
volume = {{694}},
year = {{2025}},
}