activity
20222026
most citedInterpretation of the light curve of GeV-TeV emission from the 2021 outburst of the recurrent nova RS Ophiuchi

13 citations · 59 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.HE2026

An extra hard spectral component peaking at sub-GeV in the prompt emission of GRB 260226A

Yi-Yun Huang, Hai-Ming Zhang, Ruo-Yu Liu +1

The prompt emission spectra of gamma-ray bursts (GRBs) have long been empirically described by the Band function over the keV--MeV range, whereas several \textit{Fermi}/LAT-detecte…

astro-ph.HE2025

Constraints on Cosmic Rays Acceleration in Bright Gamma-ray Bursts with Observations of Fermi

Xing-Fu Zhang, Ruo-Yu Liu, Hai-Ming Zhang +3

Gamma-ray bursts (GRBs) are widely suggested as potential sources of ultrahigh-energy cosmic rays (UHECRs). The kinetic energy of the jets dissipates, leading to the production of…

astro-ph.HE2025★ 1 cited

Detection of a new GeV source in the outer region of the Coma cluster: a signature of external accretion shock ?

Xiao-Bin Chen, Kai Wang, Yi-Yun Huang +4

The supersonic flow motions associated with infall of baryonic gas toward sheets and filaments, as well as cluster mergers, produces large-scale shock waves. The shocks associated…

astro-ph.HE2025★ 5 cited

A two-hump spectrum in the prompt emission of GRB 240825A

Hai-Ming Zhang, Zi-Qi Wang, Cui-Yuan Dai +4

An extra hard spectral component that extends to GeV energies, in additional to the typical sub- MeV Band component, appears in several gamma-ray burst (GRBs) detected by Fermi Lar…

astro-ph.HE2024★ 9 cited

Ultrahigh-Energy Gamma-ray Emission Associated with Black Hole-Jet Systems

The LHAASO Collaboration, Zhen Cao, Felix Aharonian +315

Black holes (BH), one of the most intriguing objects in the universe, can manifest themselves through electromagnetic radiation initiated by the accretion flow. Some stellar-mass B…

astro-ph.HE2023★ 12 cited

GRB 221009A: revealing a hidden afterglow during the prompt emission phase with Fermi-GBM observations

Hai-Ming Zhang, Yi-Yun Huang, Ruo-Yu Liu +1

Recently, LHAASO reported the detection of brightest-of-all-time GRB 221009A, revealing the early onset of a TeV afterglow. However, there is no evidence of afterglow emission at s…

astro-ph.HE2023★ 11 cited

Constraints on the intergalactic magnetic field strength from -ray observations of GRB 221009A

Yi-Yun Huang, Cui-yuan Dai, Hai-Ming Zhang +2

Characteristics of the cascade gamma-ray signal resulting from very-high-energy gamma-ray sources, such as gamma-ray bursts, can be used to constrain the strength and structure of…

astro-ph.HE2022★ 8 cited

Detection of GeV emission from an ultra-long gamma-ray burst with the Fermi Large Area Telescope

Yi-Yun Huang, Hai-Ming Zhang, Kai Yan +2

GRB 220627A, detected by Fermi Gamma-ray Burst Monitor (GBM), shows two episodes of gamma-ray emission, which are separated by a {700} s long quiescent phase. Due to similar…

astro-ph.HE2022★ 13 cited

Interpretation of the light curve of GeV-TeV emission from the 2021 outburst of the recurrent nova RS Ophiuchi

Jian-He Zheng, Yi-Yun Huang, Ze-Lin Zhang +3

Nova outbursts take place in binary star systems comprising a white dwarf (WD) and either a low-mass Sun-like star (classical novae) or, a red giant. GeV gamma-ray emission has bee…