2 papers
astro-ph.SR2026
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 $…