activity
20152026
most citedMost Lithium-rich Low-mass Evolved Stars Revealed as Red Clump stars by Asteroseismology and Spectroscopy

59 citations · 214 across the 18 of their papers we have counts for

collaborators
Showing 2024Show all

5 papers · 1 filter

astro-ph.GA20246 cited

A Modified Initial Mass Function of the First Stars with Explodability Theory under Different Enrichment Scenarios

Ruizheng Jiang, Gang Zhao, Haining Li +1

The most metal-poor stars record the earliest metal enrichment triggered by Population III stars. By comparing observed abundance patterns with theoretical yields of metal-free sta…

astro-ph.GA2024

Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. III. Dynamically Tagged Groups and Chemodynamical Properties

Ruizhi Zhang, Tadafumi Matsuno, Haining Li +9

Very metal-poor (VMP) stars record the signatures of early accreted galaxies, making them essential tools for unraveling the early stages of Galaxy formation. Understanding the ori…

astro-ph.GA20245 cited

Detection of the actinide Th in an r-process-enhanced star with accretion origin

Xing Qianfan, Zhao Gang, Aoki Wako +4

The thorium and six second-peak r-process element (56<Z<72) abundances are determined for the alpha-poor star LAMOST J1124+4535 based on a high-resolution spectrum obtained with th…

astro-ph.GA20241 cited

Determining Stellar Elemental Abundances from DESI Spectra with the Data-Driven Payne

Meng Zhang, Maosheng Xiang, Yuan-Sen Ting +8

Stellar abundances for a large number of stars are key information for the study of Galactic formation history. Large spectroscopic surveys such as DESI and LAMOST take median-to-l…

astro-ph.SR2024

Spectacular nucleosynthesis from early massive stars

Alexander P. Ji, Sanjana Curtis, Nicholas Storm +39

Stars formed with initial mass over 50 Msun are very rare today, but they are thought to be more common in the early universe. The fates of those early, metal-poor, massive stars a…