activity
20192024
most citedA wide star-black-hole binary system from radial-velocity measurements

200 citations · 344 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2024★ 33 cited

A potential mass-gap black hole in a wide binary with a circular orbit

Wang Song, Zhao Xinlin, Feng Fabo +28

Mass distribution of black holes identified through X-ray emission suggests a paucity of black holes in the mass range of 3 to 5 solar masses. Modified theories have been devised t…

astro-ph.SR2023

Near-Infrared Ca II Triplet As An Stellar Activity Indicator: Library and Comparative Study

Xin Huang, Yu-JI He, ZhongRui Bai +11

We have established and released a new stellar index library of the Ca II Triplet, which serves as an indicator for characterizing the chromospheric activity of stars. The library…

astro-ph.SR2023

Orbital parameters for an ELM white dwarf with a white dwarf companion: LAMOST J033847.06+413424.2

Hailong Yuan, Zhenwei Li, Zhongrui Bai +14

Double white dwarf systems are of great astrophysical importance in the field of gravitational wave and Type Ia supernova. While the binary fraction of CO core white dwarf is about…

astro-ph.SR2023★ 1 cited

Wide binaries with white dwarf or neutron star companions discovered from Gaia DR3 and LAMOST

Xinlin Zhao, Huijun Mu, Song Wang +12

Gaia DR3 mission has identified and provided about 440,000 binary systems with orbital solutions, offering a valuable resource for searching binaries including a compact component.…

astro-ph.IM2023★ 17 cited

An in-depth exploration of LAMOST Unknown spectra based on density clustering

Haifeng Yang, Xiaona Yin, Jianghui Cai +6

LAMOST (Large Sky Area Multi-Object Fiber Spectroscopic Telescope) has completed the observation of nearly 20 million celestial objects, including a class of spectra labeled `Unkno…

astro-ph.HE2022★ 20 cited

Discovery of one neutron star candidate from radial velocity monitoring

Hailong Yuan, Song Wang, Zhongrui Bai +8

We report the discovery of one possible neutron star binary ( 0.8666 day) by using the LAMOST low-resolution spectroscopic data. The visible companion is a late A-ty…

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★ 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.SR2022★ 14 cited

Binaries with possible compact components discovered from the LAMOST Time-Domain Survey of four 2 plates

Li Xue, Wang Song, Zhao Xinlin +4

Time-domain (TD) spectroscopic data from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) can provide accurate and high-cadence radial velocities (RVs). In th…

astro-ph.SR2022★ 8 cited

ELM of ELM-WD: An extremely low mass hot star discovered in LAMOST survey

Hailong Yuan, Zhenwei Li, Zhongrui Bai +7

The Extremely Low Mass White Dwarfs (ELM WDs) and pre-ELM WDs are helium core white dwarfs with mass . Evolution simulations show that a lower mass limit for EL…

astro-ph.SR2019★ 200 cited

A wide star-black-hole binary system from radial-velocity measurements

Jifeng Liu, Haotong Zhang, Andrew W. Howard +52

All stellar mass black holes have hitherto been identified by X-rays emitted by gas that is accreting onto the black hole from a companion star. These systems are all binaries with…