activity
20232026
most citedEinstein Probe discovery of EP240408a: a peculiar X-ray transient with an intermediate timescale

21 citations · 26 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.SR2026

A superflare of BP Tau simultaneously caught by EP X-ray and TESS optical observations

Xingyu Zhou, Mingjun Liu, Gregory J. Herczeg +10

Multiwavelength observations of stellar flares trace the activity of different components of the stars' outer atmosphere, providing insight into their interactions. In the present…

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.HE2025★ 2 cited

Accretion with two-phase gas supply and its application in black hole X-ray binaries

Yilong Wang, B. F. Liu, Mingjun Liu

Accretion in black hole X-ray binaries is commonly believed to be supplied by the Roche lobe overflow or the stellar wind. The former is thought to form a geometrically thin disc w…

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

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.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.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.IM2024★ 2 cited

Long-term stability of scientific X-ray CMOS detectors

Mingjun Liu, Qinyu Wu, Zhixing Ling +3

In recent years, complementary metal-oxide-semiconductor (CMOS) sensors have been demonstrated to have significant potential in X-ray astronomy, where long-term reliability is cruc…

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.IM2024

Radiation Effects on Scientific CMOS Detectors for X-ray Astronomy: II. Total Ionizing Dose Irradiation

Mengxi Chen, Zhixing Ling, Mingjun Liu +6

Complementary metal-oxide-semiconductor (CMOS) detectors are a competitive choice for current and upcoming astronomical missions. To understand the performance variations of CMOS d…

astro-ph.HE2023

Constraining the X-ray radiation origin of 3C 273 in the low state by polarization

Mingjun Liu, Wenda Zhang, Weimin Yuan

3C 273 is one of the nearest high-luminosity quasars. Although classified as a blazar, 3C 273 also has some features in Seyferts, whose X-ray may originate from the corona. Since b…

astro-ph.IM2023

Radiation effects on scientific CMOS sensors for X-ray astronomy: I. proton irradiation

Mingjun Liu, Zhixing Ling, Qinyu Wu +5

Complementary metal-oxide-semiconductor (CMOS) sensors are a competitive choice for future X-ray astronomy missions. Typically, CMOS sensors on space astronomical telescopes are ex…