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Chengyuan Wu

31 papers hereh-index 10218 citations38 works total

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

author position
  • first author10
  • middle author19
  • last author2

Across the 31 of 31 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR24
  • astro-ph.HE6
  • astro-ph.IM1
same name
  • Chengyuan Wu — 11 papers, h 6
  • Chengyuan Wu — 9 papers, h 2
  • Chengyuan Wu — 2 papers
  • Chengyuan Wu — 2 papers, h 3
  • Chengyuan Wu — 1 paper, h 29

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
20152026
most citedUltra-compact X-ray binaries with He star companions

44 citations · 378 across the 31 of their papers we have counts for

collaborators
Showing 2025Show all

3 papers · 1 filter

astro-ph.SR2025

Evolution Models of CO WD -- AGB Star Merger Remnants

Chengyuan Wu, Heran Xiong, Shi Jia +2

Common envelope evolution is a critical but still poorly understood phase in binary evolution. It plays a key role in forming close binaries such as hot subdwarfs, double white dwa…

astro-ph.SR2025

Helium-burning blue large-amplitude pulsators: A Population Study with BPASS

Zhengyang Zhang, Conor M. Byrne, Chengyuan Wu +1

Blue Large-Amplitude Pulsators (BLAPs) are a class of radially pulsating stars with effective temperatures ranging from 20,000 to 35,000 K and pulsation periods between 7 and 75 mi…

astro-ph.SR2025★ 2 cited

Binary Evolution Pathways to Blue Large-Amplitude Pulsators: Insights from HD 133729

Zhengyang Zhang, Chengyuan Wu, Xianfei Zhang +2

Blue Large-Amplitude Pulsators (BLAPs) represent a recently identified class of pulsating stars distinguished by their short pulsation periods (2−60 minutes) and asymmetric lig…

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