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most citedA possible formation scenario of the Gaia ID 3425577610762832384: inner binary merger inside a triple common envelope

5 citations · 9 across the 12 of their papers we have counts for

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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

Orbital Parameters of 665 Double-lined Spectroscopic Binaries in the LAMOST Medium-Resolution Survey

Sufen Guo, Mikhail Kovalev, Jiao Li +9

The period, mass ratio, eccentricity, and other orbital parameters are fundamental for investigating binary star evolution. However, the number of binaries with known orbital param…

astro-ph.SR2025★ 3 cited

The Impact of Neutrino Magnetic Moments on the Evolution of the Helium Flash and Lithium-Rich Red Clump Stars

Xizhen Lu, Chunhua Zhu, Guoliang Lü +3

The detection of the neutrino magnetic moment (NMM,) is one of the most significant challenges in physics. The additional energy loss due to NMM can significantly influence th…

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…

astro-ph.SR2025★ 5 cited

A possible formation scenario of the Gaia ID 3425577610762832384: inner binary merger inside a triple common envelope

Zhuowen Li, Xizhen Lu, Guoliang Lü +3

Recently, an identified non-interacting black hole (BH) binary, Gaia ID 3425577610762832384 (hereafter G3425), contains a BH (3.6 M) falling within the mass gap and…

astro-ph.SR2024

A possible formation scenario of the Gaia BH1: inner binary merger in triple systems

Zhuowen Li, Chunhua Zhu, Xizhen Lu +5

Based on astrometric measurements and spectral analysis from DR3, two quiescent black hole (BH) binaries, BH1 and BH2, have been identified. Their origins remain cont…