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Xiangcun Meng

43 papers hereh-index 15762 citations61 works total

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

author position
  • sole author1
  • first author25
  • middle author13
  • last author4

Across the 43 of 43 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR35
  • astro-ph.HE4
  • astro-ph3
  • astro-ph.CO1
same name
  • Xiangcun Meng — 12 papers, h 2
  • Xiangcun Meng — 8 papers, h 1
  • Xiangcun Meng — 1 paper

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
20072026
most citedEvolving to Type Ia Supernovae with Short Delay Times

107 citations · 894 across the 42 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

4 papers · 1 filter

astro-ph.HE2019★ 8 cited

High-velocity feature as the indicator of the stellar population of Type Ia supernovae

Xiangcun Meng

Although type Ia supernovae (SNe Ia) are very useful in many astrophysical fields, their exact nature is still unclear, e.g. the progenitor and explosion models. The high-velocity…

astro-ph.HE2018★ 26 cited

Subdwarf B stars as possible surviving companions in Type Ia supernova remnants

Xiangcun Meng, Jiao Li

Although type Ia supernovae (SNe Ia) are so important in many astrophysical fields, a debate on their progenitor model is still endless. Searching the surviving companion in a supe…

astro-ph.HE2018★ 5 cited

Why Are Peculiar Type Ia Supernovae More Likely to Show the Signature of a Single-degenerate Model?

Xiangcun Meng, Zhanwen Han

Although type Ia supernovae (SNe Ia) are very useful in many astrophysical fields, their exact progenitor nature is still unclear. A basic method to distinguish the different proge…

astro-ph.HE2017★ 12 cited

A Polarization Sequence for Type Ia Supernovae?

Xiangcun Meng, Jujia Zhang, Zhanwen Han

Early polarization observations on Type Ia supernovae (SNe Ia) may reveal the geometry of supernova ejecta, and then put constraints on their explosion mechanism and their progenit…

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