4 citations · 5 across the 4 of their papers we have counts for
4 papers
Dynamical Mass Loss at the End of TP-AGB stars
Yingzhen Cui, Song Wang, Xiangcun Meng +3
The thermally pulsating asymptotic giant branch (TP-AGB) phase plays a key role in the evolution of low- to intermediate-mass stars, driving mass loss that influences their final s…
Irradiation-Driven Formation of Supersoft X-ray Sources Following Classical Novae
Weitao Zhao, Xiangcun Meng, Yingzhen Cui +1
Supersoft X-ray sources (SSSs) are characterized by persistent thermonuclear burning on the surfaces of white dwarfs (WDs).The standard model requires high mass transfer rates of $…
Irradiation-driven mass transfer for massive companion stars in supersoft X-rays sources
Weitao Zhao, Xiangcun Meng, Yingzhen Cui
Supersoft X-ray sources (SSSs) have been proposed as one of the progenitors for Type Ia supernovae. However, the exact origin of the quasi-periodic variability in the optical light…
A robust model for the origin of optical quasi-periodic variability in supersoft X-ray sources
Weitao Zhao, Xiangcun Meng, Yingzheng Cui +1
Supersoft X-ray sources (SSSs) are known as possible progenitors of Type Ia supernovae. The quasi-periodic variability has been detected in the optical light curves of SSSs. Howeve…