activity
20232026
most citedA potential mass-gap black hole in a wide binary with a circular orbit

33 citations · 71 across the 22 of their papers we have counts for

collaborators

25 papers

astro-ph.HE2026

Observational evidence of black hole event horizon from ultra-compact X-ray binaries

Qian-Qi Ma, Wei-Min Gu, Shan-Shan Weng +1

The event horizon is the most crucial feature that distinguishes black hole (BH) from all other objects in the universe. However, since no radiation can escape from the event horiz…

astro-ph.SR2026

A Sample of Long-Period Binaries with Dormant Compact-Object Candidates from LAMOST DR13 MRS and Gaia DR3

Junxing Zhou, Wei-Min Gu

Identifying dormant compact objects in non-interacting binaries is crucial for constraining the hidden population of stellar remnants. We present a systematic search for long-perio…

astro-ph.HE2026

A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap

Tian Huang, Xizhen Lu, Guoliang Lü +8

Observations of binary black hole (BBH) mergers detected by LIGO -- such as GW170729, GW190620, GW190706, GW230107, GW230820, and GW230928 -- feature high effective spins and prima…

astro-ph.HE2026

Hunting for Compact Object Binaries from eRASS1 Optical Counterparts through ZTF Time-domain Photometry and Multi-wavelength Surveys

Xin-Yu Fang, Hao-Bin Liu, Wei-Min Gu

Capitalizing on the eRASS1 optical counterpart catalog, we conduct a systematic census of compact object binary (COB) candidates, with a primary focus on X-ray binaries (XRBs), by…

astro-ph.HE2026

The Evolution of Cataclysmic Variables Under Various Magnetic Braking Prescriptions

Wen-Shi Tang, Xiang-Dong Li, Zhe Cui +2

Recent studies revealed discrepancies between observations and the predictions of the standard magnetic braking (MB). Although alternative models have been broadly discussed in neu…

astro-ph.SR2026

Searching for Contact Binaries with LAMOST and TESS

Ting Wu, Jin-Zhong Liu, Senyu Qi +4

Contact binaries (CBs) serve as fundamental laboratories for studying complex stellar interactions, including mass transfer, tidal effects, and angular momentum loss. In this work,…

astro-ph.SR2026

Probing Compact Objects in Wide-Orbit Binaries with Joint LAMOST LRS and MRS

Hao-Bin Liu, Wei-Min Gu

Wide-orbit binaries serve as crucial laboratories for understanding stellar evolution and identifying quiescent compact objects. In this work, we search for compact objects in wide…

astro-ph.SR2026

SED and Galactic kinematic diagnostics for dormant BH/NS binary candidates

Qian-Yu An, Wei-Min Gu

The third data release of the Gaia mission (Gaia DR3) has enabled large-scale searches for dormant black hole and neutron star binaries with stellar companions at AU-scale separati…

astro-ph.SR2026★ 1 cited

Classical Be Stars and Classical Be Star Binaries from LAMOST DR12

Qian-Yu An, Wei-Min Gu, Zhi-Xiang Zhang

Classical Be (CBe) stars are rapidly rotating B-type stars with Balmer emission lines that originated from the decretion disks surrounding them in their spectra. Accounting for $\s…

astro-ph.HE2025★ 1 cited

The first extragalactic ultra-compact X-ray binary : a candidate black hole-white dwarf system

Qian-Qi Ma, Jiachang Zhang, Wei-Min Gu +3

M31 UCXB-1 is one of the brightest X-ray point sources in the bulge of M31, with a peak X-ray luminosity $ L_{\mathrm{0.5-10 \: keV}} = 2.9^{+0.2}_{-0.2} \times 10^{38} \: \mathrm{…

astro-ph.SR2025

A Study of Cataclysmic Variables from the eFEDS Survey

Rui Wang, Wei-Min Gu, Zhi-Xiang Zhang +3

We present 17 cataclysmic variables (CVs) obtained from the crossmatch between the Sloan Digital Sky Survey (SDSS) and eROSITA Final Equatorial Depth Survey (eFEDS), including 8 kn…

astro-ph.HE2025★ 2 cited

Explanation of the Mass Distribution of Binary Black Hole Mergers

Lei Li, Guoliang Lv, Chunhua Zhu +5

Gravitational wave detectors are observing an increasing number of binary black hole (BBH) mergers, revealing a bimodal mass distribution of BBHs, which hints at diverse formation…

astro-ph.GA2025

Discovery of Repeating Transitions in 16 Changing-look Active Galactic Nuclei

Qian Dong, Zhi-Xiang Zhang, Wei-Min Gu +5

The repeating changing-look active galactic nuclei (RCL AGNs) exhibit multiple appearances and disappearances of broad emission lines (BELs), whose underlying mechanism remains a p…

astro-ph.SR2025★ 1 cited

A Be star-black hole binary with a wide orbit from LAMOST time-domain survey

Qian-Yu An, Yang Huang, Wei-Min Gu +21

Binary systems consisting of an early type star and a black hole (BH) are crucial for understanding various astrophysical phenomena, particularly the origins of detected gravitatio…

astro-ph.HE2025

Searching for Accreting Compact Object Binaries in SRG/eROSITA eRASS1

Hao-Bin Liu, Wei-Min Gu, Yongqi Lu +2

Compact object binaries with accreting white dwarfs, neutron stars, or black holes are crucial for understanding accretion physics. In this study, we identify accreting compact obj…

astro-ph.GA2025

A Sandwich Model for Changing-Look AGNs

Qian-Qi Ma, Wei-Min Gu, Zhen-Yi Cai +4

The spectral variability of changing-look active galactic nuclei (CL-AGNs) occurred on timescales of years to tens of years, posing a significant challenge to the standard thin dis…

astro-ph.SR2025

A Sample of Extreme Eclipsing Binaries with Accretion Disks from LAMOST and ZTF

Jiangxinxin Zhuang, Zhi-Xiang Zhang, Wei-Min Gu +1

Extreme eclipsing binaries may harbor peculiar physical properties. In this work, we aim to identify a sample of such systems by selecting binaries with pronounced eclipsing light…

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.GA2024★ 3 cited

Newly Discovered Changing-look Active Galactic Nuclei from SDSS and LAMOST Surveys

Qian Dong, Zhi-Xiang Zhang, Wei-Min Gu +2

Changing-look Active Galactic Nuclei (CL AGNs) exhibit drastic variations in broad emission lines (BELs), the mechanism of which remains unclear. Expanding the sample of CL AGNs is…

astro-ph.SR2024

Two Dynamically Discovered Compact Object Candidate Binary Systems from LAMOST Low-resolution Survey

Senyu Qi, Wei-Min Gu, Zhi-Xiang Zhang +3

We report two binary systems, LAMOST J035540+381550 (hereafter J035540) and LAMOST J035916+400732 (hereafter J035916), identified through the Large Sky Area Multi-Object Fiber Spec…

astro-ph.SR2024★ 1 cited

A Sample of Compact Object Candidates in Single-lined Spectroscopic Binaries from LAMOST Medium Resolution Survey

Hao-Bin Liu, Wei-Min Gu, Zhi-Xiang Zhang +3

The stellar spectra from LAMOST Medium Resolution Survey can be used to search for compact objects in binaries. The LAMOST DR10 catalog includes > 980, 000 targets with multiple me…

astro-ph.GA2024★ 13 cited

A new timescale-mass scaling for the optical variation of active galactic nuclei across the intermediate-mass to supermassive scales

Zhen-Bo Su, Zhen-Yi Cai, Mouyuan Sun +3

Variability of active galactic nuclei (AGNs) has long been servicing as an essential avenue of exploring the accretion physics of black hole (BH). There are two commonly used metho…

astro-ph.SR2024

The hidden companion in J1527: a 0.69 solar-mass white dwarf?

Zhi-Xiang Zhang, Hao-Bin Liu, Tuan Yi +2

Finding nearby neutron stars can probe the supernova and metal-enrichment histories near our Solar system. Recently, Lin et al. 2023 reported an exciting neutron star candidate, 2M…

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.…