Results 101 to 110 of about 6,070 (203)
Gamma-ray flares from pulsar wind nebulae in the Large Magellanic Cloud [PDF]
B. A. Nizamov, M. S. Pshirkov
openalex +1 more source
A Catalog of Pulsar X-Ray Filaments
We present the first Chandra X-ray Observatory (CXO) catalog of “pulsar X-ray filaments,” or “misaligned outflows.” These are linear, synchrotron-radiating features powered by ultrarelativistic electrons and positrons that escape from bow shock pulsars ...
Jack T. Dinsmore, Roger W. Romani
doaj +1 more source
X-Ray Polarization Detection of the Pulsar Wind Nebula in G21.5–0.9 with IXPE
We present the X-ray polarization observation of G21.5−0.9, a young Galactic supernova remnant (SNR), conducted with the Imaging X-ray Polarimetry Explorer (IXPE) in 2023 October, with a total livetime of approximately 837 ks.
Niccolò Di Lalla +100 more
doaj +1 more source
The density of the Earth’s middle and upper atmosphere is an important parameter in Earth science and plays a critical role in the design, operation, and orbital determination of low Earth orbit spacecraft.
Hao-Hui Zhang +10 more
doaj +1 more source
A GeV-TeV particle component and the barrier of cosmic-ray sea in the Central Molecular Zone. [PDF]
Huang X, Yuan Q, Fan YZ.
europepmc +1 more source
Statistical correlation studies of astrophysical objects with H.E.S.S. data [PDF]
Recent advances in the instrumentation to observe very high energy (VHE) gamma rays have made the discovery of many new sources possible, most of them being discovered in the Galactic plane survey of H.E.S.S., an array of imaging atmospheric Cherenkov ...
Wenig, I.
core +1 more source
Solution to the sigma problem of pulsar wind nebulae [PDF]
Oliver Porth +2 more
openalex +1 more source
Magnetic fields and relativistic electrons fill entire galaxy cluster. [PDF]
Botteon A +15 more
europepmc +1 more source
STUDY OF FOUR YOUNG TeV PULSAR WIND NEBULAE WITH A SPECTRAL EVOLUTION MODEL [PDF]
Shuta J. Tanaka +3 more
openalex +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

