Results 91 to 100 of about 47,603 (141)
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
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X‐Ray Spectra of Young Pulsars and Their Wind Nebulae: Dependence on Spin‐Down Energy Loss Rate [PDF]
E. V. Gotthelf
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Galactic Gamma-Ray Diffuse Emission at TeV Energies with HAWC Data
Galactic gamma-ray diffuse emission (GDE) is emitted by cosmic rays (CRs), ultra-relativistic protons, and electrons, interacting with gas and electromagnetic radiation fields in the interstellar medium.
R. Alfaro+80 more
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Millimeter-wave Imaging of Pulsar Wind Nebulae [PDF]
D. C.‐J. Bock, B. M. Gaensler
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Polarization in the inner region of pulsar wind nebulae [PDF]
N. Bucciantini+3 more
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The Boomerang Nebula is a bright radio and X-ray pulsar wind nebula (PWN) powered by an energetic pulsar, PSR J2229+6114. It is spatially coincident with one of the brightest ultrahigh-energy (UHE; ≥100 TeV) gamma-ray sources, LHAASO J2226+6057.
Xiao-Bin Chen+3 more
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A search for pulsar wind nebulae using pulsar gating
B. M. Gaensler+3 more
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Diffusive synchrotron radiation from pulsar wind nebulae [PDF]
Gregory D. Fleishman, M. F. Bietenholz
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