collaborators

9 papers

astro-ph.HE2025

A comprehensive study of time delay between optical/near-infrared and X-ray emissions in black hole X-ray binaries

Dizhan Du, Bei You, Zhen Yan +3

We conducted a comprehensive study of daily delays using multi-wavelength data from a sample of well-studied black hole X-ray binaries, specifically focusing on the sources GX 339-…

astro-ph.GA2024

Exploring variation of double-peak broad-line profile in strongly variable AGNs

Jiancheng Wu, Qingwen Wu, Kaixing Lu +4

The geometry and kinematics of the broad-line region (BLR) in AGNs are still unclear, which is crucial for studying the physics and evolution of supermassive black holes (SMBHs) an…

astro-ph.HE2024

Magnetic Flux Transport in Advection Dominated Accretion Flow Towards the Formation of Magnetically Arrested Disk

Jia-Wen Li, Xinwu Cao

The magnetically arrested disks (MADs) have attracted much attention in recent years. The formation of MADs are usually attributed to the accumulation of a sufficient amount of dyn…

astro-ph.HE2024

A physical model for radio and X-ray correlation in black hole X-ray binaries

Yiheng Jiang, Shanshan Li, Xinwu Cao +3

A tight correlation between the radio and X-ray emission in the hard state of black hole X-ray binaries (BHXRBs) indicates an intrinsic disc-jet connection in stellar black hole ac…

astro-ph.GA2024

Do all the quasars and high-excitation radio galaxies (HERGs) in the 3CRR catalog contain a magnetically arrested disk (MAD)?

Shuang-Liang Li, Wenwen Zuo, Xinwu Cao

Based on the magnetization, an accretion disk with large-scale magnetic field can be separated into either standard and normal evolution (SANE) or magnetically arrested disk (MAD),…

astro-ph.HE2024

The delayed radio emission in the black hole X-ray binary MAXI J1348630

Bei You, Shuai-kang Yang, Zhen Yan +2

We explore the coupling between the accretion flow and the jet in black hole X-ray binary (BHXRB) MAXI J1348-630 by analyzing the X-ray and radio observations during its 2019 outbu…

astro-ph.GA2024

Instability of Circumnuclear Gas Supply as An Origin of "Changing-look" Phenomenon of Supermassive Blackholes

J. Wang, D. W. Xu, Xinwu Cao +3

The origin of the "Changing-look" (CL) phenomenon in supermassive black holes (SMBHs) remains an open issue. This study aims to shed light on this phenomenon by focusing on a sampl…

astro-ph.HE2024

Exploring the properties of photosphere and emission lines for tidal disruption events based on the global solution of slim disk and winds

Yuehua Zhang, Qingwen Wu, Jiancheng Wu +2

The theoretical debris supply rate from a tidal disruption of stars can exceed about one hundred times of the Eddington accretion rate for a supermassive black…

astro-ph.CO2024

Magnetically arrested disks in FR I radio galaxies

Han He, Bei You, Ning Jiang +5

A sample of 17 FR I radio galaxies constructed from the 3CR catalog, which is characterized by edge-darkened radio structures, is studied. The optical core luminosities derived fro…