553 citations · 2.6k across the 67 of their papers we have counts for
67 papers
Can dwarf novae produce type Ia supernovae?
Ruijie Li, Chengyuan Wu, Zhibin Dai +1
Accreting white dwarfs (WDs) are considered one of the most promising progenitor candidates for Type Ia supernovae (SNe Ia). Dwarf novae (DNe), a subclass of cataclysmic variables…
A born ultramassive white dwarf-hot subdwarf super-Chandrasekhar candidate
Changqing Luo, Jiao Li, Chuanjie Zheng +16
Although supernovae is a well-known endpoint of an accreting white dwarf, alternative theoretical possibilities has been discussing broadly, such as the accretion-induced collapse…
Evolution of double oxygen-neon white dwarf merger remnant
Chengyuan Wu, Heran Xiong, Zhanwen Han +1
Double white dwarf (WD) merger process and their post-merger evolution are important in many fields of astronomy, such as supernovae, gamma-ray bursts, gravitational waves, etc. Th…
The progenitors of Type Ia supernovae with asymptotic giant branch donors
Luhan Li, Dongdong Liu, Bo Wang
Type Ia supernovae (SNe Ia) are among the most energetic events in the Universe. They are excellent cosmological distance indicators due to the remarkable homogeneity of their ligh…
Evolving ONe WD+He WD systems to ultra-compact X-ray binaries
Dongdong Liu, Bo Wang
It has been proposed that accretion-induced collapse (AIC) of massive white dwarfs (WDs) is an indispensable path for the formation of neutron star (NS) binaries. Although there ar…
Evolution of the post merger remnants from the coalescence of oxygen-neon and carbon-oxygen white dwarf pairs
Chengyuan Wu, Heran Xiong, Jie Lin +4
Although multidimensional simulations have investigated the processes of double WD mergers, post-merger evolution only focused on the carbon-oxygen (CO) WD or helium (He) WD merger…