Discovery of a Metal-poor Red Giant Star with the Highest Ultralithium Enhancement

Abstract We present the discovery of 2MASS J05241392−0336543 (hereafter J0524−0336), a very metal-poor ([Fe/H] = −2.43 ± 0.16), highly r -process-enhanced ([Eu/Fe] = +1.34 ± 0.10) Milky Way halo field red giant star, with an ultrahigh Li abundance of A (Li, 3D, NLTE) = 6.15 ± 0.25 and [Li/Fe] = +7.64 ± 0.25, respectively. This makes J0524−0336 the most lithium-enhanced giant star discovered to date. We present a detailed analysis of the star’s atmospheric stellar parameters and chemical abundance determinations. Additionally, we detect indications of infrared excess, as well as observe variable emission in the wings of the H α absorption line across multiple epochs, indicative of a potential enhanced mass-loss event with possible outflows. Our analysis reveals that J0524−0336 lies either between the bump and the tip of the red giant branch (RGB), or on the early asymptotic giant branch (e-AGB). We investigate the possible sources of lithium enrichment in J0524−0336, including both internal and external sources. Based on current models and on the observational evidence we have collected, our study shows that J0524−0336 may be undergoing the so-called lithium flash that is expected to occur in low-mass stars when they reach the RGB bump and/or the e-AGB.

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Publication Details

Journal
The Astrophysical Journal
Published
2024-09-26
DOI
https://doi.org/10.3847/1538-4357/ad6004
Citations
4
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
1.33

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article

Discovery of a Metal-poor Red Giant Star with the Highest Ultralithium Enhancement

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4 citations
The Astrophysical Journal
Stellar, planetary, and galactic studies
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article

Discovery of a Metal-poor Red Giant Star with the Highest Ultralithium Enhancement

Terese T. Hansen, Timothy C. Beers, Jeremy Kowkabany, Erika M. Holmbeck, Ian U. Roederer, C. Charbonnel, Anna Frebel, Rana Ezzeddine, Vinicius M. Placco, Charli M. Sakari, Yangyang Li, Zoe Hackshaw, Ella Xi Wang
article en
4 citations

Abstract

Abstract We present the discovery of 2MASS J05241392−0336543 (hereafter J0524−0336), a very metal-poor ([Fe/H] = −2.43 ± 0.16), highly r -process-enhanced ([Eu/Fe] = +1.34 ± 0.10) Milky Way halo field red giant star, with an ultrahigh Li abundance of A (Li, 3D, NLTE) = 6.15 ± 0.25 and [Li/Fe] = +7.64 ± 0.25, respectively. This makes J0524−0336 the most lithium-enhanced giant star discovered to date. We present a detailed analysis of the star’s atmospheric stellar parameters and chemical abundance determinations. Additionally, we detect indications of infrared excess, as well as observe variable emission in the wings of the H α absorption line across multiple epochs, indicative of a potential enhanced mass-loss event with possible outflows. Our analysis reveals that J0524−0336 lies either between the bump and the tip of the red giant branch (RGB), or on the early asymptotic giant branch (e-AGB). We investigate the possible sources of lithium enrichment in J0524−0336, including both internal and external sources. Based on current models and on the observational evidence we have collected, our study shows that J0524−0336 may be undergoing the so-called lithium flash that is expected to occur in low-mass stars when they reach the RGB bump and/or the e-AGB.

The Astrophysical JournalVol. 973(2)
University of Geneva (CH), Institut de Recherche en Astrophysique et Planétologie (FR)
National Science Foundation, National Aeronautics and Space Administration, National Computational Infrastructure, Australian Government, Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements, European Space Agency, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, Nuclear Safety and Security Commission, Vetenskapsrådet, Center for Undergraduate Research and Scholarship, Bowling Green State University, National Cancer Institute, Astrophysics Division
Openalex Percentile: Top 19%
Stellar, planetary, and galactic studies
1.33
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