activity
20242026
collaborators

6 papers

astro-ph.HE2026

A fast X-ray transient with chromatic flares: signatures of violent collisions induced by late-time central engine reactivation

Shao-Yu Fu, Cui-Yuan Dai, Ai-Ling Wang +57

Extragalactic Fast X-ray Transients (EFXTs) represent an emerging class of high-energy phenomena characterized by X-ray outbursts lasting from tens to hundreds of seconds. However,…

astro-ph.HE2026

Multimessenger Prospects for Low-Luminosity Gamma-Ray Bursts: Joint Neutrino and X-Ray Observations

Wenkang Lian, He Gao, Shunke Ai +1

Low--luminosity gamma-ray bursts (LLGRBs) are promising candidates for high-energy neutrinos, yet no coincident neutrino events have been detected so far. Recent advances in X-ray…

astro-ph.SR2025

An axisymmetric shock breakout indicated by prompt polarized emission from the type II supernova 2024ggi

Yi Yang, Xudong Wen, Lifan Wang +18

The death of massive stars is triggered by an infall-induced bounce shock that disrupts the star. How such a shock is launched and propagates through the star is a decade-long puzz…

astro-ph.HE2024

Multiple rebrightenings in the optical afterglow of GRB 210731A: evidence for an asymmetric jet

Jin-Da Li, He Gao, Shunke Ai +1

The broadband afterglow of Gamma-ray bursts (GRBs) is usually believed to originate from the synchrotron radiation of electrons accelerated by the external shock of relativistic je…

astro-ph.HE2024

Polarization of gamma-ray burst afterglows in the context of non-axisymmetric structured jets

Jin-Da Li, He Gao, Shunke Ai +1

As the most energetic explosion in the universe, gamma-ray bursts (GRBs) are usually believed to be generated by relativistic jets. Some mechanisms (e.g. internal non-uniform magne…

astro-ph.HE2024

Engine-fed Kilonovae (Mergernovae) -- II. Radiation

Shunke Ai, He Gao, Bing Zhang

The radioactive power generated by materials within the ejecta of a binary-neutron-star (BNS) merger powers an optical transient known as a kilonova. When the central remnant of a…