Samyaday Choudhury
The VMC survey – XLIV: Mapping metallicity trends in the large magellanic cloud using near-infrared passbands
Choudhury, Samyaday; de Grijs, Richard; Bekki, Kenji; Cioni, Maria-Rosa L; Ivanov, Valentin D; Van Loon, Jacco Th; Miller, Amy E; Niederhofer, Florian; Oliveira, Joana M; Ripepi, Vincenzo; Sun, Ning-Chen; Subramanian, Smitha
Authors
Richard de Grijs
Kenji Bekki
Maria-Rosa L Cioni
Valentin D Ivanov
Jacobus Van Loon j.t.van.loon@keele.ac.uk
Amy E Miller
Florian Niederhofer
Joana Maria Oliveira j.oliveira@keele.ac.uk
Vincenzo Ripepi
Ning-Chen Sun
Smitha Subramanian
Abstract
We have derived high-spatial-resolution metallicity maps covering ~105 deg2 across the Large Magellanic Cloud (LMC) using near-infrared passbands from the VISTA Survey of the Magellanic Clouds. We attempt to understand the metallicity distribution and gradients of the LMC up to a radius of ~ 6 kpc. We identify red giant branch (RGB) stars in spatially distinct Y, (Y - Ks) colour–magnitude diagrams. In any of our selected subregions, the RGB slope is used as an indicator of the average metallicity, based on calibration to metallicity using spectroscopic data. The mean LMC metallicity is [Fe/H] = -0.42 dex (s[Fe/H] = 0.04 dex). We find the bar to be mildly metal-rich compared with the outer disc, showing evidence of a shallow gradient in metallicity (-0.008 ± 0.001 dex kpc-1) from the galaxy’s centre to a radius of 6 kpc. Our results suggest that the LMC’s stellar bar is chemically similar to the bars found in large spiral galaxies. The LMC’s radial metallicity gradient is asymmetric. It is metal-poor and flatter towards the southwest, in the direction of the Bridge. This hints at mixing and/or distortion of the spatial metallicity distribution, presumably caused by tidal interactions between the Magellanic Clouds.
Citation
Choudhury, S., de Grijs, R., Bekki, K., Cioni, M. L., Ivanov, V. D., Van Loon, J. T., …Subramanian, S. (2021). The VMC survey – XLIV: Mapping metallicity trends in the large magellanic cloud using near-infrared passbands. Monthly Notices of the Royal Astronomical Society, 507(4), 4752-4763. https://doi.org/10.1093/mnras/stab2446
Journal Article Type | Article |
---|---|
Acceptance Date | Aug 19, 2021 |
Online Publication Date | Aug 30, 2021 |
Publication Date | 2021-11 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 507 |
Issue | 4 |
Pages | 4752-4763 |
DOI | https://doi.org/10.1093/mnras/stab2446 |
Keywords | stars: abundances, Hertzsprung-Russell and colour-magnitude diagrams, galaxies: abundanes, Local Group, Magellanic Clouds |
Publisher URL | https://academic.oup.com/mnras/article-abstract/507/4/4752/6359721?redirectedFrom=fulltext |
Files
2108.10529.pdf
(4.5 Mb)
PDF
Publisher Licence URL
https://creativecommons.org/licenses/by-nc/4.0/
You might also like
The Detection of Deuterated Water in the Large Magellanic Cloud with ALMA
(2022)
Journal Article
The VMC survey. XLV. Proper motion of the outer LMC and the impact of the SMC
(2022)
Journal Article
The VMC survey - XLVI. Stellar proper motions in the centre of the Large Magellanic Cloud
(2022)
Journal Article
The first detection of deuterated water toward extragalactic hot cores with ALMA
(2021)
Journal Article
Downloadable Citations
About Keele Repository
Administrator e-mail: research.openaccess@keele.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 © 2024
Advanced Search