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20122026
most citedFast Radio Bursts: Collisions between Neutron Stars and Asteroids/Comets

125 citations · 1.4k across the 63 of their papers we have counts for

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Showing astro-ph.HEShow all

58 papers · 1 filter

astro-ph.HE2026

Constraining the Supernova Remnant Environment of FRB 190520B with Dispersion Measure and Scattering Timescale

Jia-Peng Wei, Chen Deng, Gwenael Giacinti +4

FRB 190520B is a repeating fast radio burst source whose large dispersion measure (DM) and temporal broadening suggest a dense and evolving local environment. In this work, we test…

astro-ph.HE2026

An Intertwined Short and Long GRB with 4-minute Separation

Liang Li, Yu Wang, Bing Zhang +19

Gamma-ray bursts (GRBs), the most energetic transients in the Universe, are traditionally classified into long-duration ( s) and short-duration ( s) events, ass…

astro-ph.HE2026

Pulse-resolved Classification and Characteristics of Long-duration GRBs with \emph{Swift}-BAT Data.I. Precursors versus Main Bursts

Liang Li, Yu Wang, Jin-Jun Geng +2

We present a systematic pulse-by-pulse analysis of 22 long-duration GRBs observed by \emph{Swift}, each exhibiting a well-separated precursor before the main burst. We compare dura…

astro-ph.HE2024

The Soft X-ray Aspect of Gamma-ray Bursts in the Einstein Probe Era

Hao-Xuan Gao, Jin-Jun Geng, Yi-Fang Liang +6

The Einstein Probe (EP) satellite, dedicated at time-domain high-energy astrophysics and multi-messenger astronomy, was recently launched and successfully put into operation. The w…

astro-ph.HE2024★ 1 cited

GRB 240529A: A Tale of Two Shocks

Tian-Rui Sun, Jin-Jun Geng, Jing-Zhi Yan +66

Thanks to the rapidly increasing time-domain facilities, we are entering a golden era of research on gamma-ray bursts (GRBs). In this Letter, we report our observations of GRB 2405…

astro-ph.HE2024

Intrinsic Pulse Widths of FRB 20121102A and Calculation of Broadening from Propagation and Instrumental Effects

Jia-Peng Wei, Yong-Feng Huang, Lang Cui +3

The pulse widths of fast radio bursts are always broadened due to the scattering of the plasma medium through which the electromagnetic wave passes. The recorded pulse width will b…