Lithium Abundances from the LAMOST Med-Resolution Survey Data Release 9

Fuente: arXiv
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Main Authors: Ding, Ming-Yi, Shi, Jian-Rong, Yan, Hong-liang, Li, Chun-Qian, Gao, Qi, Chen, Tian-Yi, Zhang, Jing-Hua, Liu, Shuai, Xie, Xiao-Jin, Tang, Yao-Jia, Zhou, Ze-Ming, Wang, Jiang-Tao
Format: Preprint
Published: 2024
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author Ding, Ming-Yi
Shi, Jian-Rong
Yan, Hong-liang
Li, Chun-Qian
Gao, Qi
Chen, Tian-Yi
Zhang, Jing-Hua
Liu, Shuai
Xie, Xiao-Jin
Tang, Yao-Jia
Zhou, Ze-Ming
Wang, Jiang-Tao
author_facet Ding, Ming-Yi
Shi, Jian-Rong
Yan, Hong-liang
Li, Chun-Qian
Gao, Qi
Chen, Tian-Yi
Zhang, Jing-Hua
Liu, Shuai
Xie, Xiao-Jin
Tang, Yao-Jia
Zhou, Ze-Ming
Wang, Jiang-Tao
contents Lithium is a fragile but crucial chemical element in the universe, exhibits interesting and complex behaviors. Thanks to the massive spectroscopic data from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) medium-resolution survey (MRS), we can investigate the lithium abundances in a large and diverse sample of stars, which could bring vital help to study the origin and evolution of lithium. In this work, we use the Li 6,707.8 Å line to derive the lithium abundance through a template-matching method. A catalog of precise lithium abundance is presented for 795,384 spectra corresponding to 455,752 stars from the LAMOST MRS Data Release (DR) 9. Comparing our results with those of external high-resolution references we find a good consistency with a typical deviation of σ A(Li) ~ 0.2 dex. We also analyze the internal errors using stars that have multiple LAMOST MRS observations, which will reach as low as 0.1 dex when the signal-to-noise ratio (S/N) of the spectra > 20. Besides, our result indicates that a small fraction of giant stars still exhibit surprisingly high amount of lithium contents, and 967 stars are identified as Li-rich giants with A(Li) > 1.5 dex, accounting for ~ 2.6% of our samples. If one takes into account the fact that nearly all stars deplete lithium during the main sequence, then the fraction of Li-rich stars may exceed 2.6% much. This new catalog covers a wide range of stellar evolutionary stages from pre-main sequence to giants, and will provide help to the further study of the chemical evolution of lithium.
format Preprint
id arxiv_https___arxiv_org_abs_2403_01815
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Lithium Abundances from the LAMOST Med-Resolution Survey Data Release 9
Ding, Ming-Yi
Shi, Jian-Rong
Yan, Hong-liang
Li, Chun-Qian
Gao, Qi
Chen, Tian-Yi
Zhang, Jing-Hua
Liu, Shuai
Xie, Xiao-Jin
Tang, Yao-Jia
Zhou, Ze-Ming
Wang, Jiang-Tao
Solar and Stellar Astrophysics
Astrophysics of Galaxies
Lithium is a fragile but crucial chemical element in the universe, exhibits interesting and complex behaviors. Thanks to the massive spectroscopic data from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) medium-resolution survey (MRS), we can investigate the lithium abundances in a large and diverse sample of stars, which could bring vital help to study the origin and evolution of lithium. In this work, we use the Li 6,707.8 Å line to derive the lithium abundance through a template-matching method. A catalog of precise lithium abundance is presented for 795,384 spectra corresponding to 455,752 stars from the LAMOST MRS Data Release (DR) 9. Comparing our results with those of external high-resolution references we find a good consistency with a typical deviation of σ A(Li) ~ 0.2 dex. We also analyze the internal errors using stars that have multiple LAMOST MRS observations, which will reach as low as 0.1 dex when the signal-to-noise ratio (S/N) of the spectra > 20. Besides, our result indicates that a small fraction of giant stars still exhibit surprisingly high amount of lithium contents, and 967 stars are identified as Li-rich giants with A(Li) > 1.5 dex, accounting for ~ 2.6% of our samples. If one takes into account the fact that nearly all stars deplete lithium during the main sequence, then the fraction of Li-rich stars may exceed 2.6% much. This new catalog covers a wide range of stellar evolutionary stages from pre-main sequence to giants, and will provide help to the further study of the chemical evolution of lithium.
title Lithium Abundances from the LAMOST Med-Resolution Survey Data Release 9
topic Solar and Stellar Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2403.01815