activity
20152026
most citedGamma-Ray Emission Produced by -process Elements from Neutron Star Mergers

25 citations · 108 across the 19 of their papers we have counts for

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Showing 2018Show all

6 papers · 1 filter

astro-ph.HE2018

A comprehensive analysis of Fermi Gamma-Ray Burst Data: IV. Spectral lag and Its Relation to Ep Evolution

Rui-Jing Lu, Yun-Feng Liang, Da-Bin Lin +6

The spectral evolution and spectral lag behavior of 92 bright pulses from 84 gamma-ray bursts (GRBs) observed by the Fermi GBM telescope are studied. These pulses can be classified…

astro-ph.HE2018

A lower occurrence rate of bright X-ray flares in SN-GRBs than GRBs: evidence of energy partitions?

Hui-Jun Mu, Wei-Min Gu, Jirong Mao +6

The occurrence rates of bright X-ray flares in z<1 gamma-ray bursts (GRBs) with or without observed supernovae (SNe) association were compared. Our Sample I: the z<1 long GRBs (LGR…

astro-ph.HE2018

Gamma-ray burst jet breaks revisited

Xiang-Gao Wang, Bing Zhang, En-Wei Liang +3

Gamma-ray Burst (GRB) collimation has been inferred with the observations of achromatic steepening in GRB light curves, known as jet breaks. Identifying a jet break from a GRB afte…

astro-ph.HE2018

GRB120729A: external shock origin for both the prompt gamma-ray emission and afterglow

Li-Ye Huang, Xiang-Gao Wang, WeiKang Zheng +7

Gamma-ray burst (GRB) 120729A was detected by Swift/BAT and Fermi/GBM, and then rapidly observed by Swift/XRT, Swift/UVOT, and ground-based telescopes. It had a single long and smo…

astro-ph.HE2018

Central Engine-Powered Bright X-ray Flares in Short Gamma-Ray Bursts: A Hint of Black Hole-Neutron Star Merger?

Hui-Jun Mu, Wei-Min Gu, Jirong Mao +3

Short gamma-ray bursts may originate from the merger of double neutron stars (NS) or that of a black hole (BH) and an NS. We propose that the bright X-ray flare related to the cent…

astro-ph.HE2018

First Electromagnetic Pulse Associated with a Gravitational-Wave Event: Profile, Duration, and Delay

Da-Bin Lin, Tong Liu, Jie Lin +3

We study the first electromagnetic pulse after the gravitational wave chirp signal, focusing on the profile and duration. It is found that the light curve, especially the steep dec…