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Bow shock and Local Bubble plasma unveiled by the scintillating millisecond pulsar J0437−4715
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Probing the Low-velocity Regime of Nonradiative Shocks with Neutron Star Bow Shocks
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Sanja Lazarević, Miroslav D. Filipović, Shi Dai, Roland Kothes, Adeel Ahmad, Rami Z. E. Alsaberi, Joel C. F. Balzan, Luke A. Barnes, William D. Cotton, Philip G. Edwards, Yjan A. Gordon, Frank Haberl, Andrew M. Hopkins, Bärbel S. Koribalski, Denis Leahy, Chandreyee Maitra, Marko Mićić, Gavin Rowell, Manami Sasaki, Nicholas F. H. Tothill, Grazia Umana and Velibor Velović Publications of the Astronomical Society of Australia 41 (2024) https://doi.org/10.1017/pasa.2024.13
The Dawes Review 11: From young to old: The evolutionary path of Pulsar Wind Nebulae
On the plerionic rectangular supernova remnants of static progenitors
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Modelling the γ-ray pulsar wind nebulae population in our galaxy
Roger W. Romani, Adam Deller, Lucas Guillemot, Hao Ding, Martijn de Vries, Chase Parker, Robert T. Zavala, Aurélien Chalumeau and Ismaël Cognard The Astrophysical Journal 930(2) 101 (2022) https://doi.org/10.3847/1538-4357/ac6263
Low-frequency Flux Density Measurements and Pulsars with GHz-peaked Spectra
3D dynamics and morphology of bow-shock pulsar wind nebulae
Maxim V Barkov, Maxim Lyutikov and Dmitry Khangulyan Monthly Notices of the Royal Astronomical Society 484(4) 4760 (2019) https://doi.org/10.1093/mnras/stz213
Modelling the bow shock Pulsar Wind Nebulae propagating through a non-uniform ISM
O D Toropina, M M Romanova and R V E Lovelace Monthly Notices of the Royal Astronomical Society 484(2) 1475 (2019) https://doi.org/10.1093/mnras/stz034
3D relativistic MHD simulations of bow-shock Pulsar Wind Nebulae with highly asymmetric geometry
Constraining Relativistic Bow Shock Properties in Rotation-powered Millisecond Pulsar Binaries
Zorawar Wadiasingh, Alice K. Harding, Christo Venter, Markus Böttcher and Matthew G. Baring The Astrophysical Journal 839(2) 80 (2017) https://doi.org/10.3847/1538-4357/aa69bf
Radio emission from Sgr A*: pulsar transits through the accretion disc
I. M. Christie, M. Petropoulou, P. Mimica and D. Giannios Monthly Notices of the Royal Astronomical Society: Letters 468(1) L26 (2017) https://doi.org/10.1093/mnrasl/slx017
THE TALE OF THE TWO TAILS OF THE OLDISH PSR J2055+2539
Martino Marelli, Daniele Pizzocaro, Andrea De Luca, Fabio Gastaldello, Patrizia Caraveo and Pablo Saz Parkinson The Astrophysical Journal 819(1) 40 (2016) https://doi.org/10.3847/0004-637X/819/1/40
Reverse shock emission driven by post-merger millisecond magnetar winds: Effects of the magnetization parameter
Modelling the interaction between relativistic and non-relativistic winds in the binary system PSR B1259−63/SS2883★- II. Impact of the magnetization and anisotropy of the pulsar wind
S. V. Bogovalov, D. Khangulyan, A. V. Koldoba, G. V. Ustyugova and F. A. Aharonian Monthly Notices of the Royal Astronomical Society 419(4) 3426 (2012) https://doi.org/10.1111/j.1365-2966.2011.19983.x
Stephen P. Reynolds, B. M. Gaensler and Fabrizio Bocchino Space Sciences Series of ISSI, Large-Scale Magnetic Fields in the Universe 39 231 (2011) https://doi.org/10.1007/978-1-4614-5728-2_9
THE BALMER-DOMINATED BOW SHOCK AND WIND NEBULA STRUCTURE OF γ-RAY PULSAR PSR J1741–2054
Roger W. Romani, Michael S. Shaw, Fernando Camilo, Garret Cotter and Gregory R. Sivakoff The Astrophysical Journal 724(2) 908 (2010) https://doi.org/10.1088/0004-637X/724/2/908
NEW X-RAY OBSERVATIONS OF THE GEMINGA PULSAR WIND NEBULA
Modelling interaction of relativistic and non-relativistic winds in binary system PSR B1259−63/SS2883 – I. Hydrodynamical limit
S. V. Bogovalov, D. V. Khangulyan, A. V. Koldoba, G. V. Ustyugova and F. A. Aharonian Monthly Notices of the Royal Astronomical Society 387(1) 63 (2008) https://doi.org/10.1111/j.1365-2966.2008.13226.x
Reconstructing the Guitar: Blowing Bubbles with a Pulsar Bow Shock Backflow
B. M. Gaensler, B. Stappers, S. Chatterjee, et al. Astrophysics and Space Science Library, How does the Galaxy Work? 315 141 (2005) https://doi.org/10.1007/1-4020-2620-X_24
New observations of the pulsar wind nebula in the supernova remnant CTB 80
T. A. Lozinskaya, V. N. Komarova, A. V. Moiseev and S. I. Blinnikov Astronomy Letters 31(4) 245 (2005) https://doi.org/10.1134/1.1896068
The Mouse that Soared: High‐Resolution X‐Ray Imaging of the Pulsar‐powered Bow Shock G359.23−0.82
B. M. Gaensler, E. van der Swaluw, F. Camilo, et al. The Astrophysical Journal 616(1) 383 (2004) https://doi.org/10.1086/424906
On the origin of the system PSR B 1757$\mathsf{-}$24/SNR G 5.4$\mathsf{-}$1.2
XMM‐NewtonObservations of PSR B1823−13: An Asymmetric Synchrotron Nebula around a Vela‐like Pulsar
B. M. Gaensler, N. S. Schulz, V. M. Kaspi, M. J. Pivovaroff and W. E. Becker The Astrophysical Journal 588(1) 441 (2003) https://doi.org/10.1086/368356
Spherically symmetric relativistic MHD simulations of pulsar wind nebulae in supernova remnants