activity
20082025
most citedThe multi-band nonthermal emission from the supernova remnant RX J1713.7-3946

20 citations · 90 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2025

Kinetic Simulations of Particle Acceleration in Relativistic Perpendicular Electron-positron Shocks with Proton Admixture

Huan Yu, Qi Xia, Jun Fang

Particle acceleration in relativistic shocks of electron-positron plasmas with proton admixture is investigated through two-dimensional (2D) particle-in-cell (PIC) simulations. The…

astro-ph.HE2025

Particle Acceleration along Magnetic Fields as the Origin of Ear-like Structures in Supernova Remnants

Huan Yu, Jun Fang

The origin of ear-like structures with two opposite lobes extending from the shell of supernova remnants (SNRs) remains a subject of active debate, with proposed mechanisms ranging…

astro-ph.HE2024

Nonthermal Acceleration of Electrons, Positrons and Protons at a Nonrelativistic Quasiparallel Collisionless Shock

Huan Yu, Qi Xia, Jun Fang

Energetic positrons have been observed in the interstellar medium, and high-energy positrons with relativistic energies up to approximately 1 TeV have been detected in Galactic cos…

astro-ph.HE2022★ 3 cited

Kinetic Simulation on Electron, Proton and Helium Acceleration in a Nonrelativistic Quasiparallel shock

Jun Fang, Qi Xia, Shiting Tian +2

In addition to electrons and protons, nonrelativistic quasiparallel shocks are expected to possess the ability to accelerate heavy ions. The shocks in supernova remnants are genera…

astro-ph.HE2021★ 6 cited

Investigating the energy distribution of the high-energy particles in the Crab nebula

Lu Wen, Ke-Yao Wu, Huan Yu +1

The Crab nebula is a prominent pulsar wind nebula (PWN) detected in multiband observations ranging from radio to very high-energy (VHE) -rays. Recently, -rays with energies a…

astro-ph.HE2020★ 17 cited

Investigating the multiband nonthermal emission of the 100 TeV source eHWC J2019368 with a pulsar wind nebula scenario

Jun Fang, Lu Wen, Huan Yu +1

eHWC J2019+368 is one of the sources emitting -rays with energies higher than 100 TeV based on the recent measurement with the High Altitude Water Cherenkov Observatory (HAWC),…

astro-ph.HE2020★ 8 cited

Investigating the morphology of the supernova remnant G349.7+00.2 in the medium with a density gradient

Jing-Wen Yan, Chun-Yan Lu, Lu Wen +2

G349.7 + 00.2 is a young Galactic supernova remnant (SNR) with a mushroom morphology in radio and X-rays, and it has been detected across the entire electromagnetic spectrum from r…

astro-ph.HE2019★ 6 cited

Numerically investigating the morphology of the supernova remnant SN 1006 in the ambient medium with a density discontinuity

Jun Fang, Jingwen Yan, Lu Wen +2

Multiband observations on the type Ia supernova remnant SN 1006 indicate peculiar properties in its morphologies of emission in the radio, optical and X-ray bands. In the hard X-ra…

astro-ph.HE2019★ 6 cited

Early acceleration of electrons and protons at the nonrelativistic quasiparallel shocks with different obliquity angles

Jun Fang, Chun-Yan Lu, Jing-Wen Yan +1

The early acceleration of protons and electrons in the nonrelativistic collisionless shocks with three obliquities are investigated through 1D particle-in-cell simulations. In the…

astro-ph.HE2018★ 11 cited

An explanation for the peculiar periphery of supernova remnant G309.2-0.6

Huan Yu, Jun Fang

Supernova remnant (SNR) G309.2-0.6 has a peculiar radio morphology with two bright ears to the southwest and northeast, although the main shell outside the ears is roughly circular…

astro-ph.HE2017★ 13 cited

An explanation of the formation of the peculiar periphery of Tycho's supernova remnant

Jun Fang, Huan Yu, Li Zhang

Tycho's supernova remnant (SNR) has a periphery which clearly deviates from spherical shape bash on the X-ray and radio observations. The forward shock from the southeast to the no…

astro-ph2008★ 20 cited

The multi-band nonthermal emission from the supernova remnant RX J1713.7-3946

J. Fang, L. Zhang, J. F. Zhang +2

Nonthermal X-rays and very high-energy (VHE) -rays have been detected from the supernova remnant (SNR) RX J1713.7-3946, and especially the recent observations with the \textit{S…