Numerically modelling the Cygnus Loop as a remnant evolved in an anisotropic cavityJun Fang, Li Zhang, Huan Yu|Monthly Notices of the Royal Astronomical Society|2016Cited by 25
Investigating the multiband non-thermal emission of the 100 TeV source eHWC J2019+368 with a pulsar wind nebula scenarioJun Fang, S. Z. Chen, Huan Yu et al.|Monthly Notices of the Royal Astronomical Society|2020Cited by 17
An explanation of the formation of the peculiar periphery of Tycho's supernova remnantJun Fang, Li Zhang, Huan Yu|Monthly Notices of the Royal Astronomical Society|2017Cited by 13
Three-dimensional magnetohydrodynamic studies of the non-thermal X-ray morphologies of SN 1006Huan Yu, Li Zhang, Pengfei Zhang et al.|Astronomy and Astrophysics|2015Cited by 10
A leptonic model for the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.svg"> <mml:mi>γ</mml:mi> </mml:math> -rays coincident with the tail region of the supernova remnant G106.3+2.7Huan Yu, Jun Fang, Lu Wen et al.|New Astronomy|2021Cited by 9