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20182024
most citedPossible Formation Scenarios of ZTF J153932.16+502738.8-A Gravitational Source Close to the Peak of LISA's Sensitivity

16 citations · 70 across the 12 of their papers we have counts for

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7 papers · 1 filter

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…

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★ 1 cited

Identifying symbiotic stars with machine learning

Yongle Jia, Sufen Guo, Chunhua Zhu +3

Symbiotic stars are interacting binary systems, making them valuable for studying various astronomical phenomena, such as stellar evolution, mass transfer, and accretion processes.…

astro-ph.SR2020★ 16 cited

Possible Formation Scenarios of ZTF J153932.16+502738.8-A Gravitational Source Close to the Peak of LISA's Sensitivity

Guoliang Lü, Chunhua Zhu, Zhaojun Wang +4

ZTF J153932.16+502738.8 (ZTFJ1539) is an eclipsing double-white-dwarf system with an orbital period of 6.91 minutes, and is a significant source of LISA detecting gravitational wav…

astro-ph.SR2019★ 6 cited

The Formation of Bimodal Dust Species in Nova Ejecta

Adili Duolikun, Chunhua Zhu, Zhaojun Wang +4

The formation of bimodal dust species (namely the silicate and amorphous carbon dust grains coexistent) in a nova eruption is an open problem. According to the nova model simulated…

astro-ph.SR2019★ 10 cited

The Formation of Bimodal Dust Species in Nova Ejecta I: Chemical Conditions

Chunhua Zhu, Helei Liu, Guoliang Lü +2

The formation of bimodal dust species (that is, both of silicate and amorphous carbon dust grains are observed in a nova eruption) in nova ejecta is still debated. Using the Module…