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

46 papers

astro-ph.HE2026

Rapid Orbital Decay of Supersoft X-Ray Source WX Cen: a Surrounding Circumbinary Disk

Zhi-Qiang Liu, Wei-Min Liu, Wen-Cong Chen

WX Cen is most likely a candidate of compact binary supersoft X-ray sources, which consists of a white dwarf (WD) and a donor star that fills the Roche lobe. Recently, this source…

astro-ph.SR2023

White Dwarf Mass Growth in Cataclysmic Variables: Roles of Dwarf Novae

Wei-Min Liu, Long Jiang, Wen-Cong Chen +1

The disc instability mechanism (DIM) is widely accepted to account for the transient behaviour of dwarf novae (DNe), which experience short outbursts separated by long quiescence.…

astro-ph.HE2023★ 12 cited

Simulations of the progenitors of black hole-neutron star gravitational wave sources

Long Jiang, Wen-Cong Chen, Thomas M. Tauris +2

Recent discoveries of gravitational wave (GW) events most likely originating from black hole (BH) + neutron star (NS) mergers reveal the existence of BH+NS binaries. The formation…

astro-ph.HE2023

Type Ia supernovae in NS+He star systems and the isolated mildly recycled pulsars

Yun-Lang Guo, Bo Wang, Cheng-Yuan Wu +3

Type Ia supernovae (SNe Ia) are successful cosmological distance indicators and important element factories in the chemical evolution of galaxies. They are generally thought to ori…

astro-ph.HE2023★ 13 cited

Black Hole Ultra-compact X-ray Binaries: Galactic Low-Frequency Gravitational Wave Sources

Ke Qin, Long Jiang, Wen-Cong Chen

In the Galaxy, close binaries with compact objects are important low-frequency gravitational wave (GW) sources. As potential low-frequency GW sources, neutron star/white dwarf (WD)…

astro-ph.HE2022★ 3 cited

On the X-ray pulsar HD 49798: a contracting white dwarf with debris disk?

Wen-Cong Chen

HD49798/RX J0648.0-4418 is a peculiar binary including a hot subdwarf of O spectral type and a compact companion in a 1.55 day orbit. According to the steady spin period derivative…