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Ying Qin

4 papers hereh-index 325 citations13 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author1

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
  • astro-ph.SR1
same name
  • Ying Qin — 9 papers
  • Ying Qin — 9 papers, h 22
  • Ying Qin — 7 papers, h 12
  • Ying Qin — 4 papers, h 11
  • Ying Qin — 3 papers, h 3
  • Ying Qin — 3 papers, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

collaborators

4 papers

astro-ph.HE2025

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.HE2025

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.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…

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 (GW230529−​181500) with component masses estimated at…

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