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Evolution of high-energy particle distribution in Supernova Remnants
Houdun Zeng, Yuliang Xin, Siming Liu
Supernova remnants (SNRs) have been considered as the dominant contributors to Galactic cosmic rays. However, the relation between high-energy particles trapped in SNRs and cosmic…
Search for GeV flare coincident with the IceCube neutrino flare
Yun-Feng Liang, Hao-Ning He, Neng-Hui Liao +3
Recently the IceCube collaboration and 15 other collaborations reported the spatial and temporal coincidence between the neutrino event IceCube-170922A and the radio-TeV activity o…
Active galactic nuclei with GeV activities and the PeV neutrino source candidate TXS 0506+056
Neng-Hui Liao, Yu-Liang Xin, Yun-Feng Liang +5
On 2017 September 22 the IceCube neutrino observatory detected a track-like, very-high-energy event (IceCube-170922A) that is spatially associated with TXS 0506+056, a quasar at a…
HESS J1640-465 -- a Gamma-ray emitting pulsar wind nebula ?
Yu-Liang Xin, Neng-Hui Liao, Xiao-Lei Guo +4
HESS J1640-465 is an extended TeV -ray source and its -ray emission whether from the shell of a supernova remnant (SNR) or a pulsar wind nebula (PWN) is still under debate. W…
Fermi Large Area Telescope detection of gamma-ray emission from the direction of supernova iPTF14hls
Qiang Yuan, Neng-Hui Liao, Yu-Liang Xin +5
The remnant of supernova explosion is widely believed to be the acceleration site of high-energy cosmic ray particles. The acceleration timescale is, however, typically very long.…