collaborators

6 papers

astro-ph.HE2026

Evolution of low-mass He stars and implications for electron-capture supernova formation in close binaries

Jun-Qian Li, Ying Qin, Zi-Yuan Wang +3

The evolution of low-mass helium (He) stars (--) with neutron-star (NS) companions in close binaries has been extensively studied, but the combined effects of…

astro-ph.HE2026

Diagnosing the Properties and Evolutionary Fates of Black Hole and Wolf-Rayet X-ray Binaries as Potential Gravitational Wave Sources for the LIGO-Virgo-KAGRA Network

Zi-Yuan Wang, Ying Qin, Georges Meynet +7

IC 10 X-1, NGC 300 X-1, and Cyg X-3 constitute a unique class of X-ray binaries in which a stellar-mass black hole (BH) accretes material from a Wolf-Rayet (WR). These systems are…

astro-ph.SR2026

Formation of black holes from He stars

Gang Long, Bo Wang, Philipp Podsiadlowski +5

Massive He stars are potential candidates of type Ib/c supernova (SN) progenitors. Understanding their final fates remains a key issue in astrophysics. In this work, we investigate…

astro-ph.HE20263 cited

Reassessing the Spin of Second-born Black Holes in Coalescing Binary Black Holes and Its Connection to the chi_eff-q Correlation

Zi-Yuan Wang, Ying Qin, Rui-Chong Hu +3

The mass ratio q and effective inspiral spin chi_eff of binary black hole (BBH) mergers in GWTC-4.0 show a weaker anti-correlation than in GWTC-3.0, motivating investigation of its…

astro-ph.HE2024

Origin of Black Hole Spin in Lower-Mass-Gap Black Hole-Neutron Star Binaries

Ying Qin, Zhen-Han-Tao Wang, Georges Meynet +8

During the fourth observing run, the LIGO-Virgo-KAGRA Collaboration reported the detection of a coalescing compact binary (GW230529181500) with component masses estimated at…

astro-ph.SR2024

Stable Case BB/BC Mass Transfer to Form GW190425-like Massive Binary Neutron Star Mergers

Ying Qin, Jin-Ping Zhu, Georges Meynet +14

On April 25th, 2019, the LIGO-Virgo Collaboration discovered a Gravitational-wave (GW) signal from a binary neutron star (BNS) merger, i.e., GW190425. Due to the inferred large tot…