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researcher

Q. Cui

6 papers hereh-index 28 citations6 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author3
  • last author1

Across the 6 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
  • astro-ph.SR2
  • nucl-th1
same name
  • Q. Cui — 10 papers, h 20
  • Q. Cui — 3 papers, h 76
  • Q. Cui — 3 papers, h 3
  • Q. Cui — 2 papers, h 7
  • Q. Cui — 1 paper, h 25
  • Q. Cui — 1 paper, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20232026
most citedCorrelation between U/Th and Pb/Os abundance ratios and its application in nuclear cosmochronology

7 citations · 9 across the 4 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2026

Membership Determination of 45 Open Clusters Beyond 3 kpc

Qian Cui, Zhihong He, Yangping Luo +1

Context. Open clusters (OCs) are fundamental tracers for studying the structure and chemical evolution of the Galactic disc. Reliable identification of cluster members, particularl…

astro-ph.GA2026★ 2 cited

Star formation in the circumgalactic high-velocity cloud Complex H

Zhihong He, Wenkang Pang, Kun Wang +2

The accretion of metal-poor gas sustains galactic star formation. In the Milky Way, this process is fueled by high-velocity clouds (HVCs), yet their fundamental properties have rem…

astro-ph.GA2023

Survey for Distant Stellar Aggregates in Galactic Disk: Detecting Two Thousand Star Clusters and Candidates, along with the Dwarf Galaxy IC10

Zhihong He, Yangping Luo, Kun Wang +5

Despite having data for over 10^9 stars from Gaia, only less than 10^4 star clusters and candidates have been discovered. Particularly, distant star clusters are rarely identified,…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.