24 citations · 126 across the 12 of their papers we have counts for
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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.…
He-star donor AM CVn stars and their progenitors as LISA sources
Wei-Min Liu, Lev Yungelson, Alexandre Kuranov
Ultracompact cataclysmic variables (CVs) of the AM CVn type are deemed to be important verification sources for the future space gravitational wave detectors such as the Laser Inte…
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…
Can friction of the nova envelope account for the extra angular momentum loss in cataclysmic variables?
Wei-Min Liu, Xiang-Dong Li
It has been shown that the rate of angular momentum loss (AML) in cataclysmic variables (CVs) below the period gap is about 2.47 times that caused by gravitational radiation, sugge…
Evolution of post-Accretion Induced Collapse Binaries: the Effect of Evaporation
Wei-Min Liu, Xiang-Dong Li
Accretion-induced collapse (AIC) is widely accepted to be one of the formation channels for millisecond pulsars (MSPs). Since the MSPs have high spindown luminosities, they can imm…
On the White Dwarf Mass Problem of Cataclysmic Variables
Wei-Min Liu, Xiang-Dong Li
Recent observations show that the white dwarfs (WDs) in cataclysmic Variables (CVs) have an average mass significantly higher than isolated WDs and WDs in post-common envelope bina…
Magnetic braking of Ap/Bp stars: an alternative formation mechanism of compact intermediate-mass binary pulsars
Wei-Min Liu, Wen-Cong Chen
It is difficult for the intermediate-mass X-ray binaries (IMXBs) evolutionary channel to form intermediate-mass binary pulsars (IMBPs) with a short orbital period (less than 3 d) v…
Evolution of neutron star + He star binaries: an alternative evolutionary channel to intermediate-mass binary pulsars
Wen-Cong Chen, Wei-Min Liu
It is difficult for intermediate-mass X-ray binaries to form compact intermediate-mass binary pulsars (IMBPs) with a short orbital-period ($\la 3 \rm d$), which have a heavy ($\ga…