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Xiang-Cun Meng

3 papers hereh-index 225 citations10 works total

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

author position
  • first author1
  • middle author1
  • last author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph.SR1

identity via Semantic Scholar / OpenAlex

activity
20232025
most citedEffect of irradiation on the spin of millisecond pulsars

4 citations · 4 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2025

The helium common-envelope wind scenario for SN 2020eyj

Xiang-Cun Meng, Philipp Podsiadlowski

SN 2020eyj is the first type Ia supernova (SN Ia) showing the signature of a compact helium-rich circumstellar material (CSM). Such a large CSM is difficult to explain in a single-…

astro-ph.SR2024

On the surface helium abundance of B-type hot subdwarf stars from the WD+MS channel of Type Ia supernovae

Rui-Jie Ji, Xiang-Cun Meng, Zheng-Wei Liu

The origin of intermediate helium (He)-rich hot subdwarfs are still unclear. Previous studies have suggested that some surviving Type Ia supernovae (SNe Ia) companions from the whi…

astro-ph.HE2023★ 4 cited

Effect of irradiation on the spin of millisecond pulsars

Shunyi Lan, Xiangcun Meng

A millisecond pulsar (MSP) is an old neutron star (NS) that has accreted material from its companion star, causing it to spin up, which is known as the recycling scenario. During t…

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