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20182026
most citedFour-hundred Very Metal-Poor Stars Studied with LAMOST and Subaru. II. Elemental abundances

120 citations · 293 across the 12 of their papers we have counts for

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6 papers · 1 filter

astro-ph.SR2026

Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae

Wenyu Xin, Ken'ichi Nomoto, Chun-Ming Yip +4

Recently discovered very metal-poor (VMP) star LAMOST J1010+2358 shows a peculiar abundance pattern that is remarkably well fit by a Pop III pair-instability supernova (PISN) of $\…

astro-ph.SR2025★ 5 cited

Abundance Pattern Fitting with Bayesian Inference: Constraining First Stars' Properties and Their Explosion Mechanism with Extremely Metal-poor Stars

Ruizheng Jiang, Haining Li, Gang Zhao +2

The abundance patterns of extremely metal-poor stars preserve a fossil record of the Universe's earliest chemical enrichment by the supernova explosions from the evolution of first…

astro-ph.SR2022★ 120 cited

Four-hundred Very Metal-Poor Stars Studied with LAMOST and Subaru. II. Elemental abundances

Haining Li, Wako Aoki, Tadafumi Matsuno +9

We present homogeneous abundance analysis of over 20 elements for 385 very metal-poor (VMP) stars based on the LAMOST survey and follow-up observations with the Subaru Telescope. I…

astro-ph.SR2022★ 29 cited

Four-hundred Very Metal-poor Stars studied with LAMOST and Subaru. I. Survey Design, Follow-up Program, and Binary Frequency

Wako Aoki, Haining Li, Tadafumi Matsuno +11

The chemical abundances of very metal-poor stars provide important constraints on the nucleosynthesis of the first generation of stars and early chemical evolution of the Galaxy. W…

astro-ph.SR2020★ 24 cited

Star Formation Timescales of the Halo Populations from Asteroseismology and Chemical Abundances

Tadafumi Matsuno, Wako Aoki, Luca Casagrande +9

We combine asteroseismology, optical high-resolution spectroscopy, and kinematic analysis for 26 halo red giant branch stars in the \textit{Kepler} field in the range of $-2.5<[\ma…

astro-ph.SR2019★ 40 cited

Evidence for the accretion origin of halo stars with an extreme r-process enhancement

Qian-Fan Xing, Gang Zhao, Wako Aoki +4

Small stellar systems like dwarf galaxies are suggested to be the main building blocks of our Galaxy by numerical simulations in Lambda CDM models. The existence of star streams li…