activity
20152024
most citedA universal energy distribution for FRB 121102

44 citations · 115 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2024

A Monte-Carlo Simulation on Resonant Scattering of X-ray Line Emission in Supernova Remnants

Yiping Li, Gao-Yuan Zhang, Yang Chen +2

Resonant scattering (RS) of X-ray line emission in supernova remnants (SNRs) may modify the observed line profiles and fluxes and has potential impact on estimating the physical pr…

astro-ph.GA2022★ 17 cited

Unusually high HCO+/CO ratios in and outside supernova remnant W49B

Ping Zhou, Gao-Yuan Zhang, Xin Zhou +10

Galactic supernova remnants (SNRs) and their environments provide the nearest laboratories to study SN feedback. We performed molecular observations toward SNR W49B, the most lumin…

astro-ph.HE2019★ 44 cited

A universal energy distribution for FRB 121102

F. Y. Wang, G. Q. Zhang

Fast radio bursts (FRBs) are milliseconds radio transients with large dispersion measures (DMs). An outstanding question is the relation between repeating FRBs and those with a sin…

astro-ph.HE2016★ 34 cited

Multi-wavelength study of the supernova remnant Kes 79 (G33.6+0.1): On its supernova properties and expansion into a molecular environment

Ping Zhou, Yang Chen, Samar Safi-Harb +4

Kes 79 (G33.6+0.1) is an aspherical thermal composite supernova remnant (SNR) observed across the electromagnetic spectrum and showing an unusual highly-structured morphology, in a…

astro-ph.HE2015★ 20 cited

GeV γ-ray Emission Detected by Fermi-LAT Probably Associated with the Thermal Composite Supernova Remnant Kesteven 41 in a Molecular Environment

Bing Liu, Yang Chen, Xiao Zhang +3

Hadron emission from supernova remnant (SNR)-molecular cloud (MC) association systems has been widely regarded as a probe of the shock-accelerated cosmic-ray protons. Here, we repo…