Results 151 to 160 of about 6,506 (234)
The gamma-ray halo around Geminga indicates significant suppression of cosmic-ray diffusion. One possible explanation for this phenomenon is the projection effect of slow diffusion perpendicular to the mean magnetic field (characterized by the diffusion ...
Junji Xia+3 more
doaj +1 more source
Polarization in the inner region of pulsar wind nebulae [PDF]
N. Bucciantini+3 more
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Study of Magnetic Field and Turbulence in the TeV Halo around the Monogem Pulsar
Magnetic fields are ubiquitous in the interstellar medium, including extended objects such as supernova remnants and diffuse halos around pulsars. Its turbulent characteristics govern the diffusion of cosmic rays and the multiwavelength emission from ...
Sunil Malik, Ka Ho Yuen, Huirong Yan
doaj +1 more source
TeV gamma-rays from the Northern sky pulsar wind nebulae [PDF]
W. Bednarek, M. Bartosik
openalex +1 more source
The supernova remnant (SNR) 0540–69.3, twin of the Crab Nebula, offers an excellent opportunity to study the continuum emission from a young pulsar and pulsar wind nebula (PWN). We present observations taken with the Very Large Telescope instruments MUSE
L. Tenhu+6 more
doaj +1 more source
Chandra Spectroscopy of Pulsars and their Wind Nebulae
E. V. Gotthelf, C. M. Olbert
openalex +2 more sources
Diffusive synchrotron radiation from pulsar wind nebulae [PDF]
Gregory D. Fleishman, M. F. Bietenholz
openalex +1 more source
Signatures of Recent Cosmic-Ray Acceleration in the High-latitude Gamma-Ray Sky. [PDF]
Jóhannesson G, Porter TA.
europepmc +1 more source
A Systematic Search for MeV–GeV Pulsar Wind Nebulae without Gamma-Ray Detected Pulsars
An increasing number of pulsar wind nebulae (PWNe) are being identified in the TeV band by ground-based Imaging Air Cherenkov Telescopes such that they constitute the dominant source class of Galactic TeV emitters.
The Fermi-LAT Collaboration+108 more
doaj +1 more source