activity
20232026
most citedA potential mass-gap black hole in a wide binary with a circular orbit

33 citations · 39 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2026

The Common Envelope Evolution Outcome. III. the Improvement of Stellar Binding Energy with the Envelope Residual

Lifu Zhang, Hongwei Ge, Dylan Hebrail +7

Common-envelope evolution (CEE) is a key process in the evolution of close binary systems. Many important astrophysical objects and evolutionary stages are closely related to CEE,…

astro-ph.SR2026

Mass-Orbital Period Distribution of Massive White Dwarfs Formed Through Stable Mass Transfer

Rizhong Zheng, Hongwei Ge, Christopher A Tout +10

White dwarfs (WDs) in binaries can form through either the stable mass-transfer process or common envelope evolution (CEE). Compared to CEE, the stable mass-transfer process can le…

astro-ph.SR2026★ 1 cited

Adiabatic Mass Loss In Binary Stars. VI. Massive Helium Binary Stars

Lifu Zhang, Hongwei Ge, Zhenwei Li +6

The stability of binary mass transfer is a critical problem for binary evolution. We systematically calculate the adiabatic mass-loss model for naked helium stars with masses rangi…

astro-ph.SR2025

The relation between helium white dwarf mass and orbital period under two types of opacity

Jian Mou, Hai-Liang Chen, Dengkai Jiang +5

Helium white dwarfs (He WDs) are end products of low-mass red giant donors in close binary systems via stable mass transfer or common envelope evolution. At the end of stable mass…

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★ 33 cited

A potential mass-gap black hole in a wide binary with a circular orbit

Wang Song, Zhao Xinlin, Feng Fabo +28

Mass distribution of black holes identified through X-ray emission suggests a paucity of black holes in the mass range of 3 to 5 solar masses. Modified theories have been devised t…

astro-ph.SR2024

Adiabatic Mass Loss in Binary Stars. V. Effects of Metallicity and Nonconservative Mass Transfer -- Application in High Mass X-ray Binaries

Hongwei Ge, Christopher Adam Tout, Xuefei Chen +5

Binary stars are responsible for many unusual astrophysical phenomena, including some important explosive cosmic events. The stability criteria for rapid mass transfer and common-e…

astro-ph.SR2024

Adiabatic Mass Loss In Binary Stars. IV. Low and Intermediate Mass Helium Binary Stars

Lifu Zhang, Hongwei Ge, Xuefei Chen +1

The unstable mass transfer situation in binary systems will asymptotically cause the adiabatic expansion of the donor star and finally lead to the common envelope phase. This proce…

astro-ph.SR2023

The Common Envelope Evolution Outcome. II. Short Orbital Period Hot Subdwarf B Binaries Reveal a Clear Picture

Hongwei Ge, Christopher A Tout, Ronald F Webbink +6

The common envelope evolution (CEE) is vital in forming short orbital period compact binaries. It covers many objects, such as double compact merging binaries, type Ia supernovae p…