Results 171 to 180 of about 11,249 (249)

Galactic Gamma-Ray Diffuse Emission at TeV Energies with HAWC Data

open access: yesThe Astrophysical Journal
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
doaj   +1 more source

Modeling the X-Ray Emission of the Boomerang Nebula and Implication for Its Potential Ultrahigh-energy Gamma-Ray Emission

open access: yesThe Astrophysical Journal
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
doaj   +1 more source

Diffusive synchrotron radiation from pulsar wind nebulae [PDF]

open access: bronze, 2007
Gregory D. Fleishman, M. F. Bietenholz
openalex   +1 more source

SNR G54.1+0.3, a PeVatron Candidate Unveiled by LHAASO

open access: yesThe Astrophysical Journal
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
doaj   +1 more source

Kilonovae. [PDF]

open access: yesLiving Rev Relativ, 2020
Metzger BD.
europepmc   +1 more source

Modeling the Saddle-like GeV–TeV Spectrum of HESS J1809–193: Gamma Rays Arising from Reverse-shocked Pulsar Wind Nebula?

open access: yesThe Astrophysical Journal
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
doaj   +1 more source

Home - About - Disclaimer - Privacy