Results 101 to 110 of about 878 (215)

High energy processes in pulsar wind nebulae

open access: yesAstrophysics and Space Science, 2007
9 pages, 1 figure, Proc.
openaire   +2 more sources

A Catalog of Pulsar X-Ray Filaments

open access: yesThe Astrophysical Journal
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
doaj   +1 more source

X-Ray Polarization Detection of the Pulsar Wind Nebula in G21.5–0.9 with IXPE

open access: yesThe Astrophysical Journal
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
doaj   +1 more source

Particle acceleration in Pulsars and Pulsar Wind Nebulae

open access: yes, 2022
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.
openaire   +1 more source

Measurement of Neutral Atmosphere Density during the Years of Increasing Solar Activity Using Insight-HXMT Data with the Earth Occultation Technique

open access: yesThe Astrophysical Journal
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
doaj   +1 more source

Magnetic fields and relativistic electrons fill entire galaxy cluster. [PDF]

open access: yesSci Adv, 2022
Botteon A   +15 more
europepmc   +1 more source

Pulsar Wind Nebulae from X-rays to VHE gamma-rays [PDF]

open access: green, 2012
Oleg Kargaltsev   +2 more
openalex   +1 more source

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