A Systematic NLTE Study of Very Metal-Poor Stars with Metallicity Down to $-4.3$ dex. II. Lithium Abundance and New Insight to the Lithium Plateau

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Main Authors: Yan, Hong-Liang, Qin, Jinxiao, Liu, Shuai, Zhou, Zeming, Zhao, Gang, Shi, Jianrong, Alexeeva, Sofya, Zhang, Huawei, Li, Haining, Chen, Huiling, Zhang, Junbo, Shen, Yufu, Aoki, Wako, Matsuno, Tadafumi, Zhao, Jingkun
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Published: 2026
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author Yan, Hong-Liang
Qin, Jinxiao
Liu, Shuai
Zhou, Zeming
Zhao, Gang
Shi, Jianrong
Alexeeva, Sofya
Zhang, Huawei
Li, Haining
Chen, Huiling
Zhang, Junbo
Shen, Yufu
Aoki, Wako
Matsuno, Tadafumi
Zhao, Jingkun
author_facet Yan, Hong-Liang
Qin, Jinxiao
Liu, Shuai
Zhou, Zeming
Zhao, Gang
Shi, Jianrong
Alexeeva, Sofya
Zhang, Huawei
Li, Haining
Chen, Huiling
Zhang, Junbo
Shen, Yufu
Aoki, Wako
Matsuno, Tadafumi
Zhao, Jingkun
contents Metal-poor stars are crucially important for understanding the early Galaxy, first stars, and the Universe. In this series of papers, we present a homogeneous non-local thermodynamic equilibrium (NLTE) abundances analysis of 12 elements for 103 very/extremely metal-poor (VMP/EMP) stars with metallicity down to $-4.3$ dex. The sample was selected from the LAMOST survey and observed by the high-resolution spectroscopy of Subaru. In this paper, we present the NLTE abundances and evolution of lithium in these stars. We report different lithium behaviors corresponding to different evolutionary stages and their signatures: 1) The Spite Plateau shows a slightly positive slope, indicating increasing lithium abundance with increasing metallicity. Most significantly, it appears to extend to lower metallicities as previously suggested, calling into question the reality of the so-called 'meltdown' at low metallicity; 2) We confirm a lithium plateau for lower red giant branch (LRGB) stars with A(Li) $= 1.13$ dex in our sample, while lithium abundance drops rapidly to A(Li)$<0.5$ as stars continue to evolve to higher stage. 3) We identify four Li-rich stars in our sample across different evolutionary stages, showing complex and multiple lithium production mechanisms in VMP/EMP stars. These findings suggest that early Galactic lithium enrichment results from a complex interplay between depletion and production processes.
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id arxiv_https___arxiv_org_abs_2605_19334
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle A Systematic NLTE Study of Very Metal-Poor Stars with Metallicity Down to $-4.3$ dex. II. Lithium Abundance and New Insight to the Lithium Plateau
Yan, Hong-Liang
Qin, Jinxiao
Liu, Shuai
Zhou, Zeming
Zhao, Gang
Shi, Jianrong
Alexeeva, Sofya
Zhang, Huawei
Li, Haining
Chen, Huiling
Zhang, Junbo
Shen, Yufu
Aoki, Wako
Matsuno, Tadafumi
Zhao, Jingkun
Solar and Stellar Astrophysics
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
Metal-poor stars are crucially important for understanding the early Galaxy, first stars, and the Universe. In this series of papers, we present a homogeneous non-local thermodynamic equilibrium (NLTE) abundances analysis of 12 elements for 103 very/extremely metal-poor (VMP/EMP) stars with metallicity down to $-4.3$ dex. The sample was selected from the LAMOST survey and observed by the high-resolution spectroscopy of Subaru. In this paper, we present the NLTE abundances and evolution of lithium in these stars. We report different lithium behaviors corresponding to different evolutionary stages and their signatures: 1) The Spite Plateau shows a slightly positive slope, indicating increasing lithium abundance with increasing metallicity. Most significantly, it appears to extend to lower metallicities as previously suggested, calling into question the reality of the so-called 'meltdown' at low metallicity; 2) We confirm a lithium plateau for lower red giant branch (LRGB) stars with A(Li) $= 1.13$ dex in our sample, while lithium abundance drops rapidly to A(Li)$<0.5$ as stars continue to evolve to higher stage. 3) We identify four Li-rich stars in our sample across different evolutionary stages, showing complex and multiple lithium production mechanisms in VMP/EMP stars. These findings suggest that early Galactic lithium enrichment results from a complex interplay between depletion and production processes.
title A Systematic NLTE Study of Very Metal-Poor Stars with Metallicity Down to $-4.3$ dex. II. Lithium Abundance and New Insight to the Lithium Plateau
topic Solar and Stellar Astrophysics
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2605.19334