activity
20242026
most citedAn extreme particle accelerator powered by pulsar PSR J1849-0001

3 citations · 3 across the 2 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2026

Ultra-high-energy -ray imprints from PeV particles accelerated by supernova remnants

Zhen Cao, F. Aharonian, Y. X. Bai +320

The quest for the origin of cosmic ray (CRs) is a fundamental issue in astrophysics. Shocks of supernova remnants (SNRs) have been considered as the dominant contributors to Galact…

astro-ph.HE20263 cited

An extreme particle accelerator powered by pulsar PSR J1849-0001

The LHAASO Collaboration

Pulsar wind nebulae (PWNe) are bubbles of relativistic particles, powered by the rotational energy loss of the central pulsars. The Crab Nebula, powered by the Milky Way's most ene…

astro-ph.HE2025

The energy structure function of fast radio bursts supports a stochastic origin model

Yi-Nan Chen, Yong-Kun Zhang, Zi-Gao Dai

The origin of fast radio bursts (FRBs) has remained a mystery up to now. There are two kinds of process invoking neutron stars as an origin of FRBs, namely inner-driven starquakes…

astro-ph.HE2025

The Extreme Faraday Effect in Fast Radio Bursts

Yu-Chen Huang, Zi-Gao Dai

Fast radio bursts (FRBs) are a type of highly-polarized, millisecond-duration electromagnetic pulses in the radio band, which are mostly produced at cosmological distances. These p…

astro-ph.HE2025

Spreading and multi-wavelength emissions of an ultra-narrow relativistic jet from GRB 221009A

Jin-Jun Geng, Ying-Kang Zhang, Hao-Xuan Gao +19

The long-term evolution of relativistic jets in gamma-ray bursts (GRBs), particularly from days to months post-burst, remains a fundamental puzzle in astrophysics. Here, we report…

astro-ph.HE2024

Time-integrated polarizations in GRB prompt phase via the Multi-window interpretation

Xu Wang, Mi-Xiang Lan, Qing-Wen Tang +2

The multi-window observations, including the light curve and the evolutions of the spectral peak energy (), the polarization degree (PD) and the polarization angle (PA), are u…