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

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Showing 2021Show all

6 papers · 1 filter

astro-ph.SR2021★ 32 cited

Novel Model of an Ultra-stripped Supernova Progenitor of a Double Neutron Star

Long Jiang, Thomas M. Tauris, Wen-Cong Chen +1

Recent discoveries of double neutron star (DNS) mergers and ultra-stripped supernovae (SNe) raise the questions of their origin and connection. We present the first 1D~model of a D…

astro-ph.HE2021★ 44 cited

Ultra-compact X-ray binaries with He star companions

Bo Wang, Wencong Chen, Dongdong Liu +5

Ultra-compact X-ray binaries (UCXBs) are low-mass X-ray binaries with hydrogen-deficient mass-donors and ultra-short orbital periods. They have been suggested to be the potential L…

astro-ph.HE2021★ 4 cited

A Strange Star Scenario for the Formation of Eccentric Millisecond Pulsar PSR J1946+3417

L. Jiang, Na Wang, Wen-Cong Chen +4

PSR J is a millisecond pulsar (MSP) with a spin period . Harbored in a binary with an orbital period days, the MSP is accompanied…

astro-ph.HE2021★ 2 cited

Influence of irradiation-driven winds on the evolution of intermediate-mass black hole X-ray binaries

Xiao-Qin Han, Long Jiang, Wen-Cong Chen

In young dense clusters, an intermediate-mass black hole (IMBH) may get a companion star via exchange encounters or tidal capture, and then evolves toward IMBH X-ray binary by the…

astro-ph.HE2021★ 7 cited

Ultra-compact binary pulsars as continuous dual-line gravitational wave sources

Wen-Cong Chen

Binary millisecond pulsars (MSPs) are detached binary systems consisting of a MSP and a He white dwarf. If the initial orbital periods of binary MSPs are less than 0.3 day, they wo…

astro-ph.SR2021★ 24 cited

On the progenitors of AM CVn stars as LISA sources: the evolved donor star channel

Wei-Min Liu, Long Jiang, Wen-Cong Chen

The space gravitational wave (GW) detector Laser Interferometer Space Antenna (LISA) that was planed to launch in the early 2030s is to detect the low-frequency GW signals in the G…