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Cited article:

High-Energy Emission from Pulsars and their Systems

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THREE-DIMENSIONAL RELATIVISTIC MAGNETOHYDRODYNAMIC SIMULATIONS OF CURRENT-DRIVEN INSTABILITY. II. RELAXATION OF PULSAR WIND NEBULA

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Large-Scale Magnetic Fields in the Universe

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High-Energy Emission from Pulsars and their Systems

Pasquale Blasi and Elena Amato
Astrophysics and Space Science Proceedings, High-Energy Emission from Pulsars and their Systems 623 (2011)
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Effective area calibration of the reflection grating spectrometers of XMM-Newton

J. S. Kaastra, C. P. de Vries, E. Costantini and J. W. A. den Herder
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Observations of ‘wisps’ in magnetohydrodynamic simulations of the Crab Nebula

N. F. Camus, S. S. Komissarov, N. Bucciantini and P. A. Hughes
Monthly Notices of the Royal Astronomical Society 400 (3) 1241 (2009)
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Non-thermal emission from relativistic MHD simulations of pulsar wind nebulae: from synchrotron to inverse Compton

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PoGOLite – A high sensitivity balloon-borne soft gamma-ray polarimeter

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Astroparticle Physics 30 (2) 72 (2008)
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FILAMENTATION INSTABILITY OF INTERACTING CURRENT SHEETS IN STRIPED RELATIVISTIC WINDS: THE ORIGIN OF LOW SIGMA?

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International Journal of Modern Physics D 17 (09) 1419 (2008)
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DeepChandraObservation of the Pulsar Wind Nebula Powered by Pulsar PSR J1846−0258 in the Supernova Remnant KES 75

C.‐Y. Ng, P. O. Slane, B. M. Gaensler and J. P. Hughes
The Astrophysical Journal 686 (1) 508 (2008)
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T. Mizuno, M. Arimoto, M. Axelsson, C. -I. Bjornsson, G. Bogaert, P. Carlson, W. Craig, Y. Fukazawa, S. Gunji, L. Hjalmarsdotter, T. Kamae, Y. Kanai, J. Kataoka, J. Katsuta, N. Kawai, M. Kiss, W. Klamra, S. Larsson, G. Madejski, C. Marini Bettolo, J. Ng, M. Pearce, F. Ryde, H. Tajima, H. Takahashi, et al.
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ECHO: a Eulerian conservative high-order scheme for general relativistic magnetohydrodynamics and magnetodynamics

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Faint X‐Ray Structure in the Crab Pulsar Wind Nebula

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