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Evolution of High-energy Electron Distribution in Pulsar Wind Nebulae
Yi-Ming Liu, Hou-Dun Zeng, Yu-Liang Xin, Si-Ming Liu and Yi Zhang Research in Astronomy and Astrophysics 24(7) 075016 (2024) https://doi.org/10.1088/1674-4527/ad50b7
Turbulent Transport Characteristics of the Particles within Pulsar Wind Nebulae 3C58 and G54.1+0.3
Non-thermal emission and spectral evolution properties of G54.1+0.3
Ji-Yang Ren, Quan-Gui Gao, Huai-Zhen Li, et al. Monthly Notices of the Royal Astronomical Society 487(4) 5781 (2019) https://doi.org/10.1093/mnras/stz1704
Dust formation in embryonic pulsar-aided supernova remnants
Conor M B Omand, Kazumi Kashiyama and Kohta Murase Monthly Notices of the Royal Astronomical Society 484(4) 5468 (2019) https://doi.org/10.1093/mnras/stz371
Multiband nonthermal radiative properties of pulsar wind nebulae
A Massive Shell of Supernova-formed Dust in SNR G54.1+0.3
Tea Temim, Eli Dwek, Richard G. Arendt, Kazimierz J. Borkowski, Stephen P. Reynolds, Patrick Slane, Joseph D. Gelfand and John C. Raymond The Astrophysical Journal 836(1) 129 (2017) https://doi.org/10.3847/1538-4357/836/1/129
The gas-to-extinction ratio and the gas distribution in the Galaxy
Hui Zhu, Wenwu Tian, Aigen Li and Mengfei Zhang Monthly Notices of the Royal Astronomical Society 471(3) 3494 (2017) https://doi.org/10.1093/mnras/stx1580
THE PROPERTIES OF THE PROGENITOR SUPERNOVA, PULSAR WIND, AND NEUTRON STAR INSIDE PWN G54.1+0.3
DEEPCHANDRAOBSERVATIONS OF THE CRAB-LIKE PULSAR WIND NEBULA G54.1+0.3 ANDSPITZERSPECTROSCOPY OF THE ASSOCIATED INFRARED SHELL
Tea Temim, Patrick Slane, Stephen P. Reynolds, John C. Raymond and Kazimierz J. Borkowski The Astrophysical Journal 710(1) 309 (2010) https://doi.org/10.1088/0004-637X/710/1/309
Arecibo HiAbsorption Measurements of Pulsars and the Electron Density at Intermediate Longitudes in the First Galactic Quadrant
J. M. Weisberg, S. Stanimirović, K. Xilouris, et al. The Astrophysical Journal 674(1) 286 (2008) https://doi.org/10.1086/523345
Improving the Angular Resolution of Coded-Mask Telescopes by Direct Demodulation