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Wen-Cong Chen

46 papers hereh-index 18997 citations71 works total

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

author position
  • sole author12
  • first author15
  • middle author12
  • last author7

Across the 46 of 46 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE30
  • astro-ph.SR11
  • astro-ph4
  • physics.optics1
same name
  • Wen-Cong Chen — 10 papers, h 4
  • Wen-Cong Chen — 5 papers, h 2
  • Wen-Cong Chen — 1 paper, h 1

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
20052026
most citedOn the progenitors of super-Chandrasekhar mass type Ia supernovae

70 citations · 763 across the 46 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2007★ 44 cited

Evolving to type Ia supernovae with long delay time

Wen-Cong Chen, Xiang-Dong Li

Recent investigations on the delay time of type Ia supernovae have set useful constraints on the progenitors of type Ia supernovae. Here we have calculated the evolution of close b…

astro-ph2006★ 38 cited

Evolution of black-hole intermediate-mass X-ray binaries: the influence of a circumbinary disc

Wen-Cong Chen, Xiang-Dong Li

Justham, Rappaport & Podsiadlowski (2006) recently suggested that black-hole low-mass X-ray binaries (BHLMXBs) with short orbital periods may have evolved from black-hole intermedi…

astro-ph2006★ 44 cited

Orbital Evolution of Algol Binaries with a Circumbinary Disk

Wen-Cong Chen, Xiang-Dong Li, Sheng-Bang Qian

It is generally thought that conservative mass transfer in Algol binaries causes their orbits to be wider, in which the less massive star overflows its Roche-lobe. The observed dec…

astro-ph2005★ 8 cited

Low Mass X-ray Binary As the Progenitor of PSR J1713+0747

Wencong Chen, Xiangdong Li, Zhenru Wang

We have calculated the evolution of low-mass X-ray binaries that leads to the formation of the binary radio pulsars like PSR J1713+0747. We show that the mass transfer is most like…

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