Laboratory disruption of scaled astrophysical outflows by a misaligned magnetic field. [PDF]
Revet G+22 more
europepmc +1 more source
Unraveling the Nature of HAWC J1844–034 with Fermi-LAT Data Analysis and Multiwavelength Modeling
The extended ultra-high-energy (UHE) gamma-ray source HAWC J1844–034 is closely associated with two other sources, HAWC J1843–032 and HWC J1846–025. Moreover, other gamma-ray observatories like HESS, LHAASO, and Tibet AS _γ have detected UHE gamma-ray ...
Sovan Boxi+2 more
doaj +1 more source
Discovery of TeV gamma-ray emission from the pulsar wind nebula 3C 58 by MAGIC
The pulsar wind nebula (PWN) 3C 58 is one of the historical very-high-energy (VHE; E>100 GeV) gamma-ray source candidates. It has been compared to the Crab Nebula due to their morphological similarities.
López-Coto Rubén
doaj +1 more source
A Spin-down Power Threshold for Pulsar Wind Nebula Generation? [PDF]
E. V. Gotthelf
openalex +1 more source
Multiband Nonthermal Radiative Properties of the Pulsar Wind Nebula CTB 87
The pulsar wind nebula CTB 87 (G74.9+1.2) is one of the sources emitting γ -rays with energies higher than 10 TeV, as measured by the Very Energetic Radiation Imaging Telescope Array System telescope.
Yunlu Gong+5 more
doaj +1 more source
PIC methods in astrophysics: simulations of relativistic jets and kinetic physics in astrophysical systems. [PDF]
Nishikawa K+3 more
europepmc +1 more source
Energy dependent γ-ray morphology in the pulsar wind nebula HESS J1825–137 [PDF]
F. Aharonian+99 more
openalex +1 more source
Special Issue "Synthetic Aperture Radar (SAR) Techniques and Applications". [PDF]
Bovenga F.
europepmc +1 more source
X‐Ray Emission from PSR J1809−1917 and Its Pulsar Wind Nebula, Possibly Associated with the TeV Gamma‐Ray Source HESS J1809−193 [PDF]
Oleg Kargaltsev, George G. Pavlov
openalex +1 more source
Diagnosing the Particle Transport Mechanism in the Pulsar Halo via X-Ray Observations
Pulsar halos (also termed “TeV halos”) are a new class of γ -ray sources in the Galaxy, which manifest as extended γ -ray emission around middle-aged pulsars, as discovered around the Geminga pulsar, the Monogem pulsar, and PSR J0622+3749 by the High ...
Qi-Zuo Wu+4 more
doaj +1 more source