activity
20182026
most citedThe nature of the Li enrichment in the most Li-rich giant star

67 citations · 105 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2026

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

Hong-Liang Yan, Jinxiao Qin, Shuai Liu +12

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 thermodynam…

astro-ph.SR2026

Lithium in Wide Binaries: Effective Temperature Governs Depletion while Rotation Plays a Minor Role

Cheng-Cheng Xie, Hai-Jun Tian, Jian-Rong Shi +1

Using a sample of 116 wide binary systems as coeval and chemically homogeneous stellar pairs, we investigate the factors governing lithium depletion in main-sequence stars. We reco…

astro-ph.SR2025

Revisiting the Li abundances of Stars with and without Detected Planets from the High Resolution Spectroscopy

Jinxiao Qin, Hong-Liang Yan, Wenyuan Cui +12

Whether the presence of planets affects the lithium (Li) abundance of their host stars is still an open question. To investigate the difference of the Li abundance between planet-h…

astro-ph.SR2024

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

Ming-Yi Ding, Jian-Rong Shi, Hong-liang Yan +9

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 Mult…

astro-ph.SR2021★ 7 cited

LTD064402+245919: A Subgiant with a 1-3 M Undetected Companion Identified from LAMOST-TD Data

Fan Yang, Bo Zhang, Richard J. Long +11

Single-line spectroscopic binaries recently contribute to the stellar-mass black hole discovery, independently of the X-ray transient method. We report the identification of a sing…

astro-ph.SR2020★ 7 cited

LAMOST/HRS Spectroscopic Analysis of Two New Li-rich Giants

Zeming Zhou, Jianrong Shi, Hongliang Yan +9

Two Li-rich candidates, TYC 1338-1410-1 and TYC 2825-596-1, were observed with the new high-resolution echelle spectrograph, LAMOST/HRS. Based on the high-resolution and high-signa…

astro-ph.SR2018★ 67 cited

The nature of the Li enrichment in the most Li-rich giant star

Hong-Liang Yan, Jian-Rong Shi, Yu-Tao Zhou +13

About one percent of giants\upcite{Brown1989} are detected to have anomalously high lithium (Li) abundances in their atmospheres, conflicting directly with the prediction of the st…

astro-ph.SR2018★ 24 cited

NLTE analysis of copper lines in different stellar populations

J. R. Shi, H. L. Yan, Z. M. Zhou +1

The copper abundances of 29 metal-poor stars are determined based on the high resolution, high signal-to-noise ratio spectra from the UVES spectragraph at the ESO VLT telescope. Ou…