activity
20232026
most citedA two-hump spectrum in the prompt emission of GRB 240825A

5 citations · 9 across the 20 of their papers we have counts for

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astro-ph.HE2024

Modeling the X-ray emission of the Boomerang nebula and implication for its potential ultrahigh-energy gamma-ray emission

Xiao-Bin Chen, Xuan-Han Liang, Ruo-Yu Liu +1

The Boomerang nebula is a bright radio and X-ray pulsar wind nebula (PWN) powered by an energetic pulsar, PSR~J2229+6114. It is spatially coincident with one of the brightest ultra…

astro-ph.HE2024

Could the neutrino emission of TXS 0506+056 come from the accretion flow of the supermassive black hole?

Qi-Rui Yang, Ruo-Yu Liu, Xiang-Yu Wang

High-energy neutrinos from the blazar TXS 0506+056 are usually thought to arise from the relativistic jet pointing to us. However, the composition of jets of active galactic nuclei…

astro-ph.HE2024

On the External Inverse Compton Scattering off the Prompt Emission in GRB 221009A

Cui-Yuan Dai, Jian-He Zheng, Xiao-Hong Zhao +2

The light curve of the TeV emission in GRB 221009A displays a smooth transition from an initial rapid rise to a slower rise and eventually a decay phase. The smooth temporal profil…

astro-ph.HE2024

Choked precessing jets in tidal disruption events and high-energy neutrinos

Qi-Rui Yang, Jian-He Zheng, Ruo-Yu Liu +1

It has been suggested that relativistic jets might have been commonly formed in tidal disruption events (TDEs), but those with relatively weak power could be choked by the surround…

astro-ph.HE2024★ 3 cited

Probing the nova shock physics with future gamma-ray observations of the upcoming outburst from T Coronae Borealis

Jian-He Zheng, Hai-Ming Zhang, Ruo-Yu Liu +2

Nova shocks behave like scaled-down supernova remnant shocks with a lifetime of only a few weeks or months, thereby providing a unique opportunity to study the dynamics of non-rela…