Results 171 to 180 of about 6,506 (234)

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

Pulsar-wind nebulae in X-rays and TeV γ-rays [PDF]

open access: green, 2010
Oleg Kargaltsev   +4 more
openalex   +1 more source

CONSTRAINING RELATIVISTIC BOW SHOCK PROPERTIES IN ROTATION-POWERED MILLISECOND PULSAR BINARIES. [PDF]

open access: yesAstrophys J, 2017
Wadiasingh Z   +4 more
europepmc   +1 more source

Recent Very-high-energy Results on Pulsars and Pulsar Wind Nebulae

open access: yesActa Physica Polonica B, Proceedings Supplement, 2022
C. Venter
semanticscholar   +1 more source

Scaled laboratory experiments explain the kink behaviour of the Crab Nebula jet. [PDF]

open access: yesNat Commun, 2016
Li CK   +28 more
europepmc   +1 more source

NuSTAR broad-band X-ray observational campaign of energetic pulsar wind nebulae in synergy with VERITAS, HAWC and Fermi gamma-ray telescopes [PDF]

open access: hybrid, 2021
Kaya Mori   +14 more
openalex   +1 more source

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