activity
20162026
most citedThe Formation of EL CVn-type Binaries

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

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Showing 2024Show all

6 papers · 1 filter

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…