collaborators

6 papers

astro-ph.SR2026

Evolution of cataclysmic variables under different magnetic braking prescriptions

Bingyao Zhou, Chunhua Zhu, Guoliang Lü +3

Context. The evolution of cataclysmic variables (CVs) - interacting binaries where a low-mass donor transfers matter to a white dwarf via an accretion disk - is critically controll…

astro-ph.SR2025

Formation of the Dormant Black Holes with Luminous Companions from Binary or Triple Systems

Zhuowen Li, Xizhen Lu, Guoliang Lü +6

Recently, a class of dormant black hole binaries with luminous companions (dBH-LC) has been observed, such as BH1, BH2, and BH3. Unlike previously discovered X-ray BH binari…

astro-ph.SR2025

The influence of rotation and metallicity on the explodability of massive stars

Renyu Luo, Chunhua Zhu, Guoliang Lü +4

During the late stages of massive stellar evolution, failed supernovae (FSN) may form through core-collapse processes. The traditional evaluation criterion 0.45, prim…

astro-ph.SR2025

The mixing of internal gravity waves and lithium production in intermediate-mass AGB stars

Zhijun Wang, Guoliang Lü, Chunhua Zhu +3

Context: Intermediate-mass asymptotic giant branch (AGB) stars influence Galactic lithium evolution by ejecting surface material (including Li) via stellar winds. Internal gravity…

astro-ph.SR2025

The neutrino luminosity and energy spectrum of nova outburst

Hao Wang, Chunhua Zhu, Guoliang Lü +4

The nova outburst can produce a large number of neutrinos, whether it is the nuclear reaction process during the explosion or the shock wave acceleration proton process. We study t…

astro-ph.SR2025

A Study of Subsurface Convection Zones of Fast Rotating Massive Stars

Xiao-long He, Guo-liang Lv, Chun-hua Zhu +6

The subsurface convective zones (CZs) of massive stars significantly influences many of their key characteristics. Previous studies have paid little attention to the impact of rota…