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Spatio-spectral-temporal modelling of two young pulsar wind nebulae
A Kundu, Jagdish C Joshi, C Venter, N E Engelbrecht, W Zhang, Diego F Torres, I Sushch and Shuta J Tanaka Monthly Notices of the Royal Astronomical Society 535(3) 2415 (2024) https://doi.org/10.1093/mnras/stae2435
Multiwavelength Investigation of γ-Ray Source MGRO J1908+06 Emission Using Fermi-LAT, VERITAS and HAWC
A. Acharyya, C. B. Adams, P. Bangale, J. T. Bartkoske, W. Benbow, J. H. Buckley, J. L. Christiansen, A. J. Chromey, A. Duerr, M. Errando, A. Falcone, Q. Feng, G. M. Foote, L. Fortson, A. Furniss, W. Hanlon, D. Hanna, O. Hervet, C. E. Hinrichs, J. Holder, T. B. Humensky, W. Jin, P. Kaaret, M. Kertzman, D. Kieda, et al. The Astrophysical Journal 974(1) 61 (2024) https://doi.org/10.3847/1538-4357/ad698d
Likely Detection of GeV γ-Ray Emission from Pulsar Wind Nebula G32.64+0.53 with Fermi-LAT
Prospects for a survey of the galactic plane with the Cherenkov Telescope Array
S. Abe, J. Abhir, A. Abhishek, F. Acero, A. Acharyya, R. Adam, A. Aguasca-Cabot, I. Agudo, A. Aguirre-Santaella, J. Alfaro, N. Alvarez-Crespo, R. Alves Batista, J.-P. Amans, E. Amato, G. Ambrosi, F. Ambrosino, E.O. Angüner, C. Aramo, C. Arcaro, L. Arrabito, K. Asano, Y. Ascasíbar, J. Aschersleben, L. Augusto Stuani, M. Backes, et al. Journal of Cosmology and Astroparticle Physics 2024(10) 081 (2024) https://doi.org/10.1088/1475-7516/2024/10/081
Turbulent Transport Characteristics of the Particles within Pulsar Wind Nebulae 3C58 and G54.1+0.3
Investigating the Multiband Nonthermal Radiative Properties of HESS J1420−607
Shiting Tian, Liancheng Zhou, Yunlu Gong, Keyao Wu, Jun Fang and Huan Yu Publications of the Astronomical Society of the Pacific 135(1049) 074503 (2023) https://doi.org/10.1088/1538-3873/ace3f8
On the plerionic rectangular supernova remnants of static progenitors
D M-A Meyer, Z Meliani, P F Velázquez, M Pohl and D F Torres Monthly Notices of the Royal Astronomical Society 527(3) 5514 (2023) https://doi.org/10.1093/mnras/stad3495
Reverberation of pulsar wind nebulae – II. Anatomy of the ‘thin-shell’ evolution
R Bandiera, N Bucciantini, J Martín, B Olmi and D F Torres Monthly Notices of the Royal Astronomical Society 520(2) 2451 (2023) https://doi.org/10.1093/mnras/stad134
Turbulent Diffusion of the Particles within Pulsar Wind Nebulae
Investigating the radiative properties of LHAASO J1908 + 0621
Keyao Wu, Liancheng Zhou, Yunlu Gong and Jun Fang Monthly Notices of the Royal Astronomical Society 519(2) 1881 (2022) https://doi.org/10.1093/mnras/stac3618
Modelling the γ-ray pulsar wind nebulae population in our galaxy
Reverberation of pulsar wind nebulae (I): impact of the medium properties and other parameters upon the extent of the compression
R Bandiera, N Bucciantini, J Martín, B Olmi and D F Torres Monthly Notices of the Royal Astronomical Society 499(2) 2051 (2020) https://doi.org/10.1093/mnras/staa2956
Exploiting morphological data from Pulsar Wind Nebulae via a spatiotemporal leptonic transport code
C van Rensburg, C Venter, A S Seyffert and Alice K Harding Monthly Notices of the Royal Astronomical Society 492(3) 3091 (2020) https://doi.org/10.1093/mnras/staa016
Towards observing reverberating and superefficient pulsar wind nebulae
Diego F Torres, Tingting Lin and Francesco Coti Zelati Monthly Notices of the Royal Astronomical Society 486(1) 1019 (2019) https://doi.org/10.1093/mnras/stz862
High energy spatially radiative properties of Vela X pulsar wind nebula
Spatially radiative properties of 3C 58 and G21.5−0.9
Fang-Wu Lu, Quan-Gui Gao, Bo-Tao Zhu and Li Zhang Monthly Notices of the Royal Astronomical Society 472(3) 2926 (2017) https://doi.org/10.1093/mnras/stx2223
A SELF-CONSISTENT AND SPATIALLY DEPENDENT MODEL OF THE MULTIBAND EMISSION OF PULSAR WIND NEBULAE
Diffusion in pulsar wind nebulae: an investigation using magnetohydrodynamic and particle transport models
O. Porth, M. J. Vorster, M. Lyutikov and N. E. Engelbrecht Monthly Notices of the Royal Astronomical Society 460(4) 4135 (2016) https://doi.org/10.1093/mnras/stw1152
THE PROPERTIES OF THE PROGENITOR SUPERNOVA, PULSAR WIND, AND NEUTRON STAR INSIDE PWN G54.1+0.3