activity
20202026
most citedMass transfer of low-mass binaries and chemical anomalies among unevolved stars in globular clusters

4 citations · 7 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2026

Double White Dwarfs with Circumbinary Disks: Evolution, Population Properties, and Gravitational Wave Signatures

Wenwu Ma, Zhenwei Li, Dylan Hebrail +5

Double white dwarfs (DWDs) are important multi-messenger sources and powerful probes of binary interaction physics. Close DWDs formed through isolated binary evolution are expected…

astro-ph.SR2026

Revealing Optically Hidden Companions to Intermediate-Mass Stripped Stars with Radial Velocities

Alexander Laroche, Maria R. Drout, Ylva Götberg +7

The recent discovery of a population of intermediate-mass helium stars (2-8 ) in the Magellanic Clouds has opened a new observational window into massive binary evol…

astro-ph.SR2025

Formation of Be stars via wind accretion: Case study on Black hole + Be star binaries

Zhenwei Li, Shi Jia, Dandan Wei +5

Be stars are rapidly rotating main-sequence (MS) stars that play a crucial role in understanding stellar evolution and binary interactions. In this letter, we propose a new formati…

astro-ph.SR2021★ 3 cited

The fractions of post-binary-interaction stars and evolved blue straggler stars on the red giant branch of globular clusters

Dandan Wei, Bo Wang, Hailiang Chen +4

The red giant branch (RGB) of globular clusters (GCs) is home to some exotic stars, which may provide clues on the formation of multiple stellar populations in GCs. It is well know…

astro-ph.SR2020★ 4 cited

Mass transfer of low-mass binaries and chemical anomalies among unevolved stars in globular clusters

Dandan Wei, Bo Wang, Xuefei Chen +3

While it is well known that mass transfer in binaries can pollute the surfaces of the accretors, it is still unclear whether this mechanism can reproduce the observed chemical inho…