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20082026
most citedFour-hundred Very Metal-Poor Stars Studied with LAMOST and Subaru. II. Elemental abundances

120 citations · 665 across the 33 of their papers we have counts for

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Showing 2022Show all

5 papers · 1 filter

astro-ph.GA2022★ 6 cited

Existence of Tidal Tails for the Globular Cluster NGC 5824

Yong Yang, Jing-Kun Zhao, Miho N. Ishigaki +5

Context. Several dynamically cold streams have been associated with certain globular clusters (GCs) based on orbital energies and angular momenta. Some of these streams are surpris…

astro-ph.GA2022★ 7 cited

Revisit NGC 5466 Tidal Stream with , SDSS/SEGUE and LAMOST

Yong Yang, Jing-Kun Zhao, Miho N. Ishigaki +5

By mining the data from EDR3, SDSS/SEGUE DR16 and LAMOST DR8, 11 member stars of the NGC 5466 tidal stream are detected and 7 of them are newly identified. To reject contami…

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.GA2022★ 32 cited

High-precision chemical abundances of Galactic building blocks. II. Revisiting the chemical distinctness of the Helmi streams

Tadafumi Matsuno, Emma Dodd, Helmer H. Koppelman +6

Context: The Helmi streams are a kinematic substructure whose progenitor is likely a dwarf galaxy. Although 20 years have passed since their discovery, it is still unclear whether…