activity
20222026
most citedA potential mass-gap black hole in a wide binary with a circular orbit

33 citations · 38 across the 5 of their papers we have counts for

collaborators

5 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★ 33 cited

A potential mass-gap black hole in a wide binary with a circular orbit

Wang Song, Zhao Xinlin, Feng Fabo +28

Mass distribution of black holes identified through X-ray emission suggests a paucity of black holes in the mass range of 3 to 5 solar masses. Modified theories have been devised t…

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…

astro-ph.SR2022★ 4 cited

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…