Results 101 to 110 of about 878 (215)
The power-law component of the X-ray emissions from pulsar-wind nebulae and their pulsars [PDF]
Jr-Yue Hsiang, Hsiang‐Kuang Chang
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Full-3D relativistic MHD simulations of bow shock pulsar wind nebulae: dynamics [PDF]
Barbara Olmi, N. Bucciantini
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High energy processes in pulsar wind nebulae
9 pages, 1 figure, Proc.
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A Catalog of Pulsar X-Ray Filaments
We present the first Chandra X-ray Observatory (CXO) catalog of “pulsar X-ray filaments,” or “misaligned outflows.” These are linear, synchrotron-radiating features powered by ultrarelativistic electrons and positrons that escape from bow shock pulsars ...
Jack T. Dinsmore, Roger W. Romani
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X-Ray Polarization Detection of the Pulsar Wind Nebula in G21.5–0.9 with IXPE
We present the X-ray polarization observation of G21.5−0.9, a young Galactic supernova remnant (SNR), conducted with the Imaging X-ray Polarimetry Explorer (IXPE) in 2023 October, with a total livetime of approximately 837 ks.
Niccolò Di Lalla +100 more
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A GeV-TeV particle component and the barrier of cosmic-ray sea in the Central Molecular Zone. [PDF]
Huang X, Yuan Q, Fan YZ.
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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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The density of the Earth’s middle and upper atmosphere is an important parameter in Earth science and plays a critical role in the design, operation, and orbital determination of low Earth orbit spacecraft.
Hao-Hui Zhang +10 more
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Magnetic fields and relativistic electrons fill entire galaxy cluster. [PDF]
Botteon A +15 more
europepmc +1 more source
Pulsar Wind Nebulae from X-rays to VHE gamma-rays [PDF]
Oleg Kargaltsev +2 more
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