698 citations · 1.7k across the 43 of their papers we have counts for
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Influence of a mass transfer stability criterion on double white dwarf populations
Zhenwei LI, Xuefei Chen, Hongwei Ge +2
Mass transfer stability is an essential issue in binary evolution. Ge et al. studied critical mass ratios for dynamically stable mass transfer by establishing adiabatic mass loss m…
A Roche Lobe-filling hot Subdwarf and White Dwarf Binary: possible detection of an ejected common envelope
Jiangdan Li, Christopher A. Onken, Christian Wolf +12
Binaries consisting of a hot subdwarf star and an accreting white dwarf (WD) are sources of gravitational wave radiation at low frequencies and possible progenitors of type Ia supe…
Evolution of AM CVn binaries with WD donors
Hai-Liang Chen, Xuefei Chen, Zhanwen Han
The evolution and stability of mass transfer of CO+He WD binaries are not well understood. Observationally they may emerge as AM CVn binaries and are important gravitational wave (…
The Common Envelope Evolution Outcome -- A Case Study on Hot Subdwarf B Stars
Hongwei Ge, Christopher A Tout, Xuefei Chen +6
Common envelope evolution (CEE) physics plays a fundamental role in the formation of binary systems, such as mergering stellar gravitational wave sources, pulsar binaries and type…
Investigating the stability of mass transfer in neutron star-helium white dwarf binaries
Hai-Liang Chen, Thomas M. Tauris, Xuefei Chen +1
Neutron star-helium white dwarf (NS+He WD) binaries are important evolutionary products of close-orbit binary star systems. They are often observed as millisecond pulsars and may c…
Formation of millisecond pulsars with long orbital periods by accretion-induced collapse of white-dwarfs
Bo Wang, Dongdong Liu, Hailiang Chen
Accretion-induced collapse (AIC) of massive white-dwarfs (WDs) has been proposed as an important way for the formation of neutron star (NS) systems. An oxygen-neon (ONe) WD that ac…