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20112026
most citedA wide star-black-hole binary system from radial-velocity measurements

200 citations · 1.2k across the 42 of their papers we have counts for

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7 papers · 1 filter

astro-ph.HE2022★ 22 cited

On the Neutron Star/Black Hole Mass Gap and Black Hole Searches

Yong Shao

Mass distribution of black holes in low-mass X-ray binaries previously suggested the existence of a mass gap between the most massive neutron stars and the le…

astro-ph.HE2022★ 20 cited

The Nearest Neutron Star Candidate in a Binary Revealed by Optical Time-domain Surveys

Ling-Lin Zheng, Mouyuan Sun, Wei-Min Gu +19

The near-Earth (within pc) supernova explosions in the past several million years can cause the global deposition of radioactive elements (e.g., Fe) on Earth. The…

astro-ph.SR2022★ 13 cited

A long-period pre-ELM system discovered from LAMOST medium-resolution survey

Zhi-Xiang Zhang, Ling-Lin Zheng, Wei-Min Gu +16

We present LAMOST~J041920.07+072545.4 (hereafter J0419), a close binary consisting of a bloated extremely low mass pre-white dwarf (pre-ELM WD) and a compact object with an orbital…

astro-ph.SR2022★ 31 cited

A dynamically discovered and characterized non-accreting neutron star -- M dwarf binary candidate

Tuan Yi, Wei-Min Gu, Zhi-Xiang Zhang +26

Optical time-domain surveys can unveil and characterize exciting but less-explored non-accreting and/or non-beaming neutron stars (NS) in binaries. Here we report the discovery of…

astro-ph.HE2022★ 22 cited

Formation of Mass-gap Black Holes from Neutron Star X-ray Binaries with Super-Eddington Accretion

Shi-Jie Gao, Xiang-Dong Li, Yong Shao

Electromagnetic and gravitational wave observations indicate that there is dearth of compact objects with mass . This so-called "mass gap" may be linked t…

astro-ph.HE2022★ 27 cited

Stable mass transfer can explain massive binary black hole mergers with a high spin component

Yong Shao, Xiang-Dong Li

Recent gravitational wave observations showed that binary black hole (BBH) mergers with massive components are more likely to have high effective spins. In the model of isolated bi…

astro-ph.HE2022★ 30 cited

A Channel to Form Fast-spinning Black Hole--Neutron Star Binary Mergers as Multi-messenger Sources

Rui-Chong Hu, Jin-Ping Zhu, Ying Qin +3

After the successful detection of a gravitational-wave (GW) signal and its associated electromagnetic (EM) counterparts from GW170817, neutron star--black hole (NSBH) mergers have…