activity
20242026
collaborators

9 papers

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

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

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

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.HE2025

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…