Particle acceleration in Pulsars and Pulsar Wind Nebulae
Lecture slides for the course "Particle acceleration in Pulsars and Pulsar Wind Nebulae" delivered by Elena Amato at the International School of Physics Enrico Fermi - Course 208 Foundations of Cosmic Ray Astrophysics.
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Galactic Cosmic Rays Throughout the Heliosphere and in the Very Local Interstellar Medium. [PDF]
Rankin JS +9 more
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PIC methods in astrophysics: simulations of relativistic jets and kinetic physics in astrophysical systems. [PDF]
Nishikawa K +3 more
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Cross Calibration of Imaging Air Cherenkov Telescopes with Fermi [PDF]
An updated model for the synchrotron and inverse Compton emission from a population of high energy electrons of the Crab Nebula is used to reproduce the measured spectral energy distribution from radio to high energy gamma-rays.
Horns, D., Meyer, M., Zechlin, H. -S.
core
Detection of Gamma-Ray Emission from the Vela Pulsar Wind Nebula with AGILE [PDF]
A. Pellizzoni +70 more
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Special Issue "Synthetic Aperture Radar (SAR) Techniques and Applications". [PDF]
Bovenga F.
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X-ray Studies of the Pulsar Wind Nebula Around PSR B0540-69 [PDF]
Robert Petre +3 more
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From Supernova to Remnant: Tracking the Evolution of the Oldest Known X-Ray Supernovae. [PDF]
Ramakrishnan V, Dwarkadas VV.
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Faint X‐Ray Structure in the Crab Pulsar Wind Nebula [PDF]
F. D. Seward +2 more
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MHD models of Pulsar Wind Nebulae [PDF]
Pulsar Wind Nebulae (PWNe) are bubbles or relativistic plasma that form when the pulsar wind is confined by the SNR or the ISM. Recent observations have shown a richness of emission features that has driven a renewed interest in the theoretical modeling of these objects.
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