4 citations · 4 across the 9 of their papers we have counts for
9 papers
EP250302a: violent shell collision in a soft-X-ray-selected GRB-like transient
Shao-Yu Fu, Cui-Yuan Dai, Ai-Ling Wang +57
The Einstein Probe opens a previously unexplored soft X-ray window onto gamma-ray bursts, filling a critical observational gap in the soft X-ray coverage of their prompt emission.…
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…
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…
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…
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…
Supernova Polarization Signals From the Interaction with a Dense Circumstellar Disk
Xudong Wen, He Gao, Yi Yang +3
There is increasing evidence that massive stars may exhibit an enhanced mass loss shortly before their termination explosion. Some of them also indicate the enhancement of their ci…
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…
On the possibility to detect gravitational waves from post-merger super-massive neutron stars with a kilohertz detector
Yikang Chen, Bin Liu, Shunke Ai +4
The detection of a secular post-merger gravitational wave (GW) signal in a binary neutron star (BNS) merger serves as strong evidence for the formation of a long-lived post-merger…
Characteristics 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 explosions in the Universe, gamma-ray bursts (GRBs) are commonly believed to be generated by relativistic jets. Recent observational evidence suggests that th…