1 citations · 1 across the 3 of their papers we have counts for
3 papers
astro-ph.SR2026★ 1 cited
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…
astro-ph.HE2025
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 $…
astro-ph.SR2024
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…