activity
20192026
most citedModeling accretion disk emission with generalized temperature profile and its effect on AGN spectral energy distribution

28 citations · 129 across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.HE2026

Multiwavelength Analysis of the Einstein Probe X-ray Transient EP240305a

Ruican Ma, Ye Li, Lian Tao +32

We report multiwavelength observations of EP240305a, an uncatalogued X-ray transient detected by the Einstein Probe on March 5, 2024. The source exhibits distinct characteristics a…

astro-ph.HE2026

Hydrodynamical simulation of wind production from hot accretion flows in tidal disruption events

Mingjun Liu, De-Fu Bu, Xiao-Hong Yang +5

Wind is a key mechanism for supermassive black hole (SMBH) feedback to their host galaxies. In tidal disruption events (TDEs), black holes spend most of their time accreting at hig…

astro-ph.HE2026

Minutes-long soft X-ray prompt emission from a compact object merger

An Li, Chen-Wei Wang, Niccolò Passaleva +75

Compact object mergers are multi-messenger sources and known progenitors of some gamma-ray bursts, bright flashes of high-energy radiation powered by a central engine, either an ac…

astro-ph.HE2025★ 1 cited

A fast powerful X-ray transient from possible tidal disruption of a white dwarf

Dongyue Li, Wenda Zhang, Jun Yang +97

Stars captured by black holes (BHs) can be torn apart by strong tidal forces, producing electromagnetic flares. To date, more than 100 tidal disruption events (TDEs) have been obse…

astro-ph.HE2025

Multiwavelength Observations of the Apparently Non-repeating FRB 20250316A

Ye Li, Hui Sun, Lei Qian +72

The physical origin of fast radio bursts (FRBs) remains uncertain. Although multiwavelength observations have been widely conducted, only Galactic FRB~20200428D is associated with…

astro-ph.HE2025

Einstein Probe Discovery of EP J182730.0-095633: A New Black Hole X-ray Binary Candidate in Faint Outburst?

Huaqing Cheng, Qingchang Zhao, L. Tao +77

Black hole X-ray binaries (candidates) currently identified in our galaxy are mainly transient sources, with the majority discovered through the detection of their X-ray outbursts.…

astro-ph.HE2025

The effectively optically thin accretion flow and its implication in supermassive black holes

Mingjun Liu, B. F. Liu, Yilong Wang +2

Based on a unified description of various accretion flows, we find a long-ignored solution - the effectively optically thin accretion flow, occurring at accretion rates around Eddi…

astro-ph.IM2025

Ground Calibration Result of the Wide-field X-ray Telescope (WXT) onboard the Einstein Probe

Huaqing Cheng, Chen Zhang, Zhixing Ling +24

We report on results of the on-ground X-ray calibration of the Wide-field X-ray Telescope (WXT) built from novel lobster-eye micro-pore optics, onboard the Einstein Probe (EP) sate…

astro-ph.HE2025

A generalized solution for advection-dominated accretion flow, standard disc, and slim disc

Mingjun Liu, B. F. Liu, Yilong Wang +2

Aiming at a general description of four basic solutions describing the accretion processes, i.e., the Shakura-Sunyaev thin disc (SSD), the Shapiro-Lightman-Eardley solution (SLE),…

astro-ph.HE2025★ 15 cited

EP241021a: a months-duration X-ray transient with luminous optical and radio emission

Shu Xinwen, Yang Lei, Yang Haonan +82

We present the discovery of a peculiar X-ray transient, EP241021a, by the Einstein Probe (EP) mission, and the results from multiwavelength follow-up observations. The transient wa…

astro-ph.HE2024

Detection of an Orphan X-ray Flare from a Blazar Candidate EP240709a with Einstein Probe

Mingjun Liu, Yijia Zhang, Yun Wang +49

Blazars are often observed to flare across multiple wavelengths. Orphan flares from blazars have been only detected a few times, providing an opportunity to understand the structur…

astro-ph.HE2024★ 21 cited

Einstein Probe discovery of EP240408a: a peculiar X-ray transient with an intermediate timescale

Wenda Zhang, Weimin Yuan, Zhixing Ling +136

We report the discovery of a peculiar X-ray transient, EP240408a, by Einstein Probe (EP) and follow-up studies made with EP, Swift, NICER, GROND, ATCA and other ground-based multi-…

astro-ph.HE2024

LEIA discovery of the longest-lasting and most energetic stellar X-ray flare ever detected

Xuan Mao, He-Yang Liu, Song Wang +40

The Lobster Eye Imager for Astronomy (LEIA) detected a new X-ray transient on 2022 November 7, identified as a superflare event occurring on a nearby K-type giant star HD 251108. T…

astro-ph.HE2024★ 1 cited

A large population of neutron star low-mass X-ray binaries with long outburst recurrence time ?

E. Meyer-Hofmeister, Huaqing Cheng, B. F. Liu

Low-mass X-ray binaries (LMXBs) with neutron stars show quite different features which depend on the rate of mass transfer from the donor star. With a high transfer rate the Z sour…

astro-ph.IM2023

Ground Calibration Result of the Lobster Eye Imager for Astronomy

Huaqing Cheng, Zhixing Ling, Chen Zhang +22

We report on results of the on-ground X-ray calibration of the Lobster Eye Imager for Astronomy (LEIA), an experimental space wide-field (18.6*18.6 square degrees) X-ray telescope…

astro-ph.HE2022★ 4 cited

A Systematic Study of the Short-Term X-ray Variability of Seyfert Galaxies I. Diversity of the X-ray Rms Spectra

Jingwei Hu, Chichuan Jin, Huaqing Cheng +1

The X-ray variability of active galactic nuclei (AGN) carries crucial information about the X-ray radiation mechanism. We performed a systematic study of the X-ray short-term (1-10…

astro-ph.HE2020★ 6 cited

The Awakening Beast in the Seyfert 1 Galaxy KUG 1141+371 I

Jiachen Jiang, Huaqing Cheng, Luigi C. Gallo +10

KUG 1141+371 is a Seyfert 1 galaxy that shows a simultaneous flux increase in the optical and UV bands in the past decade. For instance, the latest Swift observation in 2019 shows…

astro-ph.HE2020★ 24 cited

Magnetic-reconnection-heated corona in active galactic nuclei: refined disc-corona model and application to broad-band radiation

Huaqing Cheng, B. F. Liu, Jieying Liu +3

A long-standing question in active galactic nucleus (AGN) research is how the corona is heated up to produce X-ray radiation much stronger than that arising from the viscous heatin…

astro-ph.HE2020★ 19 cited

Multiwavelength Study of an X-ray Tidal Disruption Event Candidate in NGC 5092

Dongyue Li, R. D. Saxton, Weimin Yuan +7

We present multiwavelength studies of a transient X-ray source, XMMSL1 J131952.3+225958, associated with the galaxy NGC 5092 at detected in the XMM-Newton SLew survey (XM…

astro-ph.HE2019★ 10 cited

The Large Amplitude X-ray Variability in NGC 7589: Possible Evidence for Accretion Mode Transition

Zhu Liu, He-Yang Liu, Huaqing Cheng +2

We report the discovery of large amplitude X-ray variability in the low luminosity AGN (LLAGN) MGC 7589, and present possible observational evidence for accretion mode transition i…

astro-ph.HE2019★ 28 cited

Modeling accretion disk emission with generalized temperature profile and its effect on AGN spectral energy distribution

Huaqing Cheng, Weimin Yuan, He-Yang Liu +3

The broadband spectral energy distribution (SED) of Active Galactic Nuclei (AGN) is investigated for a well-selected sample composed of Seyfert 1 galaxies observed simultaneou…