activity
20162026
most citedThe Formation of EL CVn-type Binaries

50 citations · 117 across the 18 of their papers we have counts for

collaborators

20 papers

astro-ph.HE2026

A Unified Solution to the Low-Mass X-ray Binary Diversity Puzzle: Saturated Magnetic Braking Coupled with Irradiation-Driven Winds

Zhu-Ling Deng, Xiang-Dong Li, Bo Wang +4

The standard magnetic braking (MB) model has long failed to explain key properties of low-mass X-ray binaries (LMXBs)---including their accretion rates, the formation of ultracompa…

astro-ph.HE2026

Supernova nucleosynthesis: a review

Shuai Zha, Yudong Luo, Zhanwen Han

Supernovae are major drivers of cosmic chemical evolution. They synthesize heavy elements and disperse them into the interstellar medium via their explosion shocks. Light elements…

astro-ph.SR2026

Stage-dependent superhump waveform evolution and non-stationary positive-superhump timing in the near-period-gap dwarf nova YZ Cancri

Zhibin Dai, Xuefei Chen, Zhanwen Han

We present a photometric and timing study of the near-period-gap SU~UMa-type dwarf nova YZ~Cancri, based on nearly continuous Transiting Exoplanet Survey Satellite (TESS) photometr…

astro-ph.SR2026

A Catalog of 45,206 Hα Emission-line Stars from LAMOST MRS DR7

Lihuan Yu, Jiangdan Li, Jinliang Wang +2

Stars that exhibit prominent emission lines in their spectra are referred to as emission-line stars, encompassing a wide range of stellar types and indicative of intriguing physica…

astro-ph.HE2025

The diverse morphology of gravitational wave signals from merging neutron-star white-dwarf binaries

Shenghua Yu, Youjun Lu, C. Simon Jeffery +6

In sufficiently compact neutron star-white dwarf (NSWD) binary systems, orbital decay means the white dwarf eventually fills its shrinking Roche lobe, initiating a phase of mass tr…

astro-ph.SR2025

A New Algol-type Binary with an Accretion disk

Tongyu He, Jiao Li, Xiaobin Zhang +10

We present a comprehensive photometric and spectroscopic analysis of the Algol-type binary \textit{Gaia} DR3 1892576067672499328. We identified the system as a spectroscopic binary…

astro-ph.HE2025★ 7 cited

The Formation of Electron-capture Supernovae: A Review

Bo Wang, Dongdong Liu, Yunlang Guo +1

It is generally believed that the electron-capture reactions happen when the oxygen-neon (ONe) cores grow in masses close to the Chandrasekhar limit, leading to the formation of ne…

astro-ph.SR2025

Enhanced magnetic activity in rapidly rotating binary stars

Jie Yu, Charlotte Gehan, Saskia Hekker +12

Stellar activity is fundamental to stellar evolution and the formation and habitability of exoplanets. The interaction between convective motions and rotation in cool stars results…

astro-ph.SR2025

Mass, Luminosity, and Stellar Age of Early-type Stars from the LAMOST Survey

Qida Li, Jianping Xiong, Jiao Li +4

Mass () and luminosity () are fundamental parameters of stars but can only be measured indirectly. Typically, effective temperature (), surface gravity (${\rm lo…

astro-ph.SR2025

Identify Main-sequence Binaries from the Chinese Space Station Telescope Survey with Machine Learning. II. Based on Gaia and GALEX

Jia-jia Li, Jian-ping Xiong, Zhi-jia Tian +3

The statistical characteristics of double main-sequence (MS) binaries are essential for investigating star formation, binary evolution, and population synthesis. Our previous study…

astro-ph.SR2025★ 4 cited

Detection of Ubiquitous Circumbinary Matter in Hot Subdwarfs Formed from Common-Envelope Ejections

Jiangdan Li, Christian Wolf, Jiao Li +7

The formation of compact binary systems is largely driven by their evolution through a common envelope (CE) phase, crucial for understanding phenomena such as type Ia supernovae an…

astro-ph.SR2025★ 2 cited

Binary Evolution Pathways to Blue Large-Amplitude Pulsators: Insights from HD 133729

Zhengyang Zhang, Chengyuan Wu, Xianfei Zhang +2

Blue Large-Amplitude Pulsators (BLAPs) represent a recently identified class of pulsating stars distinguished by their short pulsation periods ( minutes) and asymmetric lig…

astro-ph.SR2024★ 5 cited

The Red Supergiant Progenitor of the Type II Supernova 2024abfl

Jingxiao Luo, Lifu Zhang, Bing-Qiu Chen +9

Linkage between core-collapse supernovae (SNe) and their progenitors is not fully understood and ongoing effort of searching and identifying the progenitors is needed. $\mathrm{SN\…

astro-ph.SR2024

Discoveries and Properties of EL CVn-type Binaries in the TESS Survey

Jianping Xiong, Zhenwei Li, Jiao Li +5

EL CVn-type systems represent a rare evolutionary stage in binary star evolution, providing ideal laboratories for investigating stable mass transfer processes and the formation of…

astro-ph.SR2024★ 6 cited

Ultraluminous X-ray sources with He star companions

Luhan Li, Bo Wang, Dongdong Liu +3

Ultraluminous X-ray sources (ULXs) are non-nuclear point-like objects observed with extremely high X-ray luminosity that exceeds the Eddington limit of a black hol…

astro-ph.SR2024★ 1 cited

A born ultramassive white dwarf-hot subdwarf super-Chandrasekhar candidate

Changqing Luo, Jiao Li, Chuanjie Zheng +16

Although supernovae is a well-known endpoint of an accreting white dwarf, alternative theoretical possibilities has been discussing broadly, such as the accretion-induced collapse…

astro-ph.HE2024★ 3 cited

Electron-capture supernovae in NS+He star systems and the double neutron star systems

Yun-Lang Guo, Bo Wang, Wen-Cong Chen +4

Electron-capture supernovae (EC-SNe) provide an alternative channel for producing neutron stars (NSs). They play an important role in the formation of double NS (DNS) systems and t…

astro-ph.SR2024★ 2 cited

Formation of millisecond pulsars with wide orbits

Bo Wang, Dongdong Liu, Yunlang Guo +4

Millisecond pulsars (MSPs) are a kind of radio pulsars with short spin periods, playing a key role in many aspects of stellar astrophysics. In recent years, some more MSPs with wid…

astro-ph.SR2017★ 37 cited

Mass retention efficiencies of He accretion onto carbon-oxygen white dwarfs and type Ia supernovae

C. Wu, B. Wang, D. Liu +1

Type Ia supernovae (SNe Ia) play a crucial role in studying cosmology and galactic chemical evolution. They are thought to be thermonuclear explosions of carbon-oxygen white dwarfs…

astro-ph.SR2016★ 50 cited

The Formation of EL CVn-type Binaries

Chen Xuefei, Maxted P. F. L., Li Jiao +1

EL CVn-type binaries contain an A-type dwarf star and a very low mass () helium white dwarf precursor (pre-He WD). Recent surveys and observations have discovered…