collaborators

5 papers

astro-ph.SR2026

A Rare Population of Intermediate-mass Helium Stars Between Hot Subdwarfs and Wolf-Rayet Stars

Gui-Yu Wang, Yong Shao, Jian-Guo He +3

Helium stars stripped of their hydrogen envelopes represent pivotal phases in binary evolution, yet their origins, particularly within the intermediate-mass range of $2-8\, M_{\odo…

astro-ph.HE2026

Formation of Recycled Pulsars in Common Envelope Binaries

Yu-Dong Nie, Yong Shao, Jian-Guo He +4

We present a systematic study of the evolution of low- and intermediate-mass X-ray binaries (L/IMXBs) consisting of a neutron star (NS) and a donor star of mass $1…

astro-ph.SR2024

Modeling High Mass X-ray Binaries to Double Neutron Stars through Common Envelope Evolution

Yu-Dong Nie, Yong Shao, Jian-Guo He +3

We present detailed evolutionary simulations of wide binary systems with high-mass () donor stars and a neutron star. Mass transfer in such binari…

astro-ph.HE2024

IC 10 X-1: A Double Black Hole Progenitor Probably Formed through Stable Mass Transfer

Gui-Yu Wang, Yong Shao, Jian-Guo He +2

IC 10 X-1 is one of close X-ray binaries containing a Wolf-Rayet donor, which can provide an evolutionary link between high-mass X-ray binaries and gravitational wave sources. It i…

astro-ph.HE2024

Constraining Mass Transfer Models with Galactic Neutron StarWhite Dwarf Binaries as Gravitational Wave Sources

Jian-Guo He, Yong Shao, Xiao-Jie Xu +1

Neutron starwhite dwarf (NSWD) binaries are one of the most abundant sources of gravitational waves (GW) in the Milky Way. These GW sources are the evolutionary products of prim…