Results 91 to 100 of about 603,420 (243)
QUASI-PERIODIC PULSATIONS IN THE GAMMA-RAY EMISSION OF A SOLAR FLARE [PDF]
V. M. Nakariakov +3 more
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Potential contribution from gamma-ray sources to the Galactic diffuse gamma rays observed above 100 TeV (sub-PeV energy range) by the Tibet AS γ experiment is an important key to interpreting recent multimessenger observations.
S. Kato +10 more
doaj +1 more source
Gamma Ray Burst afterglow and prompt-afterglow relations: An overview [PDF]
M. G. Dainotti, R Del Vecchio
openalex +1 more source
A Discussion on the Origin of the Sub-PeV Galactic Gamma-Ray Emission
Galactic diffuse gamma-ray flux measured by the Tibet AS γ experiment and the total Galactic gamma-ray flux measured by the Large High Altitude Air Shower Observatory (LHAASO) are found to be consistent, within the statistical and systematic ...
S. Kato +18 more
doaj +1 more source
Ultrafast gamma-ray line emission driven by laser-accelerated ion beams
The Monte Carlo code Geant4 is used to demonstrate ultrafast gamma-ray line emission from the 12C +12C reaction driven by laser-accelerated ion beams.
Yong Yu, Baifei Shen
doaj +1 more source
Gravitationally lensed orphan afterglows of gamma-ray bursts [PDF]
Hao-Xuan Gao +9 more
openalex +1 more source
Spectroscopy of the Host Galaxy of the Gamma-Ray Burst 980703 [PDF]
S. G. Djorgovski +13 more
openalex +1 more source
X-ray absorption evolution in gamma-ray bursts: intergalactic medium or evolutionary signature of their host galaxies [PDF]
R. L. C. Starling +7 more
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Double Neutron Star Mergers and Short Gamma-ray Bursts: Long-lasting High-energy Signatures and Remnant Dichotomy [PDF]
Kohta Murase +17 more
openalex +1 more source
In 2021, RS Ophiuchi was the first nova to be detected in the very-high-energy (TeV) gamma-ray domain, directly testifying to efficient acceleration of charged particles up to at least the TeV range at the nova shock.
Vo Hong Minh Phan +4 more
doaj +1 more source

