activity
20182026
most citedMonitoring the Morphology of M87* in 2009-2017 with the Event Horizon Telescope

67 citations · 177 across the 21 of their papers we have counts for

collaborators
Showing 2024Show all

6 papers · 1 filter

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

Simulations on the collision between debris stream and outer dusty torus: a possible channel for forming fast-rise and long-delayed radio outburst in tidal disruption events

Xiangli Lei, Qingwen Wu, Hui Li +6

The geometrically thick dusty torus structure is believed to exist in the nuclear region of galaxies (especially in active galactic nuclei, AGNs). The debris stream from a tidal di…

astro-ph.IM2024★ 30 cited

First Very Long Baseline Interferometry Detections at 870μm

Alexander W. Raymond, Sheperd S. Doeleman, Keiichi Asada +276

The first very long baseline interferometry (VLBI) detections at 870m wavelength (345GHz frequency) are reported, achieving the highest diffraction-limited angular resolutio…

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.GA2024

The Interaction Between Stars and Past AGN Disk: Possible Explanation for the Kinematic Distributions of S-stars in the Galactic Center

Xiao Fan, Qingwen Wu, Jiancheng Wu +3

The presence of young stars, aged around several million years and situated within the range of pc from our Galactic center raises a question about their origins and…

astro-ph.HE2024

The weakness of soft X-ray intensity: possible physical reason for weak line quasars

Jiancheng Wu, Qingwen Wu, Chichuan Jin +8

Weak-line quasars (WLQs) are a notable group of active galactic nuclei (AGNs) that show unusually weak UV lines even though their optical-UV continuum shapes are similar to those o…