Results 171 to 180 of about 6,506 (234)
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]
Oleg Kargaltsev+4 more
openalex +1 more source
CONSTRAINING RELATIVISTIC BOW SHOCK PROPERTIES IN ROTATION-POWERED MILLISECOND PULSAR BINARIES. [PDF]
Wadiasingh Z+4 more
europepmc +1 more source
Relativistic Nonthermal Particle Acceleration in Two-Dimensional Collisionless Magnetic Reconnection. [PDF]
Uzdensky DA.
europepmc +1 more source
Citation-based clustering of publications using CitNetExplorer and VOSviewer. [PDF]
van Eck NJ, Waltman L.
europepmc +1 more source
Recent Very-high-energy Results on Pulsars and Pulsar Wind Nebulae
C. Venter
semanticscholar +1 more source
Scaled laboratory experiments explain the kink behaviour of the Crab Nebula jet. [PDF]
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]
Kaya Mori+14 more
openalex +1 more source