Results 171 to 180 of about 11,249 (249)
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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TeV gamma-rays from the Northern sky pulsar wind nebulae [PDF]
W. Bednarek, M. Bartosik
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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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Signatures of Recent Cosmic-Ray Acceleration in the High-latitude Gamma-Ray Sky. [PDF]
Jóhannesson G, Porter TA.
europepmc +1 more source
Diffusive synchrotron radiation from pulsar wind nebulae [PDF]
Gregory D. Fleishman, M. F. Bietenholz
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SNR G54.1+0.3, a PeVatron Candidate Unveiled by LHAASO
Recently, the LHAASO Collaboration reported the first very-high-energy gamma-ray catalog, containing 90 TeV sources. Among these sources, 1LHAASO J1929+1846u is located 0 $\mathop{.}\limits^{\unicode{x000b0}}$ 3 west of SNR G54.1+0.3 and also lies within
Yihan Shi, Yudong Cui, Lili Yang
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The evolution of pulsar wind nebulae (PWNe) could be expected to leave imprints in gamma rays. We suggest that the intriguing GeV–TeV spectral energy distribution (SED) of HESS J1809–193 and Fermi-LAT source J1810.3–1925e is very likely to be the gamma ...
Jiaxu Sun+4 more
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Chandra Spectroscopy of Pulsars and their Wind Nebulae
E. V. Gotthelf, C. M. Olbert
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