Results 141 to 150 of about 8,336 (234)

Laboratory disruption of scaled astrophysical outflows by a misaligned magnetic field. [PDF]

open access: yesNat Commun, 2021
Revet G   +22 more
europepmc   +1 more source

Unraveling the Nature of HAWC J1844–034 with Fermi-LAT Data Analysis and Multiwavelength Modeling

open access: yesThe Astrophysical Journal
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

open access: yesEPJ Web of Conferences, 2016
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

Multiband Nonthermal Radiative Properties of the Pulsar Wind Nebula CTB 87

open access: yesThe Astrophysical Journal
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

Energy dependent γ-ray morphology in the pulsar wind nebula HESS J1825–137 [PDF]

open access: bronze, 2006
F. Aharonian   +99 more
openalex   +1 more source

Diagnosing the Particle Transport Mechanism in the Pulsar Halo via X-Ray Observations

open access: yesThe Astrophysical Journal
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

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