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most citedExplanation of the Mass Distribution of Binary Black Hole Mergers

2 citations · 3 across the 11 of their papers we have counts for

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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.HE2025★ 2 cited

Explanation of the Mass Distribution of Binary Black Hole Mergers

Lei Li, Guoliang Lv, Chunhua Zhu +5

Gravitational wave detectors are observing an increasing number of binary black hole (BBH) mergers, revealing a bimodal mass distribution of BBHs, which hints at diverse formation…

astro-ph.SR2025★ 1 cited

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

New symbiotic stars or candidates in LAMOST low resolution spectra

Yabing Zhao, Sufen Guo, Guoliang Lv +3

Symbiotic stars are among the most crucial binary systems for studying binary star interactions and Type Ia supernova progenitors. Based on the unique observational characteristics…

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

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…