output
20112024
most citedLi-rich and super Li-rich giants produced by element diffusion

12 citations

11 papers

astro-ph.SR2024★ 9 cited

Novae: An Important Source of Lithium in the Galaxy

Jun Gao, Chunhua Zhu, Guoliang Lü +4

The source of the Galactic Lithium (Li) has long been a puzzle. With the discovery of Li in novae, extensive research has been conducted. However, there still exists a significant…

astro-ph.SR2024★ 11 cited

The population synthesis of Wolf-Rayet stars involving binary merger channels

Zhuowen Li, Chunhua Zhu, Guoliang Lü +5

Wolf-Rayet stars (WRs) are very important massive stars. However, their origin and the observed binary fraction within the entire WR population are still debated. We investigate so…

astro-ph.SR2023★ 6 cited

Hydrogen-free Wolf-Rayet stars: Helium stars with envelope-inflation structure and rotation

Xizhen Lu, Chunhua Zhu, Helei Liu +3

Observations have shown that the effective temperature of hydrogen-free Wolf-Rayet (WR) stars is considerably lower than that of the standard model, which means that the radius of…

astro-ph.SR2022★ 12 cited

Li-rich and super Li-rich giants produced by element diffusion

Jun Gao, Chunhua Zhu, Jinlong Yu +4

Context. About 0.2-2% of giant stars are Li-rich, whose lithium abundance (A(Li)) is higher than 1.5 dex. Among them, near 6% are super Li-rich with A(Li) exceeding 3.2 dex. Meanwh…

math.CO2018

A generalization of Noel-Reed-Wu Theorem to signed graphs

Wei Wang, Jianguo Qian

Let be a signed graph where two edges joining the same pair of vertices with opposite signs are allowed. The zero-free chromatic number of is the minimum even inte…

math.CO2018

Chromatic-choosability of hypergraphs with high chromatic number

Wei Wang, Jianguo Qian

It was conjectured by Ohba and confirmed recently by Noel et al. that, for any graph , if then . This indicates that the graphs with high chroma…