Results 71 to 80 of about 706 (178)

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

Nat Commun, 2021
Revet G, Khiar B, Filippov E, Argiroffi C, Béard J, Bonito R, Cerchez M, Chen SN, Gangolf T, Higginson DP, Mignone A, Olmi B, Ouillé M, Ryazantsev SN, Skobelev IY, Safronova MI, Starodubtsev M, Vinci T, Willi O, Pikuz S, Orlando S, Ciardi A, Fuchs J.   +22 more
europepmc   +1 more source

Proper motion, spectra, and timing of PSR J1813-1749 using <i>Chandra</i> and <i>NICER</i>. [PDF]

Mon Not R Astron Soc, 2020
Ho WCG, Guillot S, Parkinson PMS, Limyansky B, Ng CY, Bejger M, Espinoza CM, Haskell B, Jaisawal GK, Malacaria C.   +9 more
europepmc   +1 more source

Detection of the Extended γ-Ray Emission around TeV Source 1LHAASO J0249+6022 with Fermi-LAT

The Astrophysical Journal
1LHAASO J0249+6022 is an extended very-high-energy γ -ray source discovered by the Large High-Altitude Air Shower Observatory. Based on nearly 16.1 yr of data from the Fermi Large Area Telescope, we report the probable γ -ray emission from 1LHAASO J0249 ...
Yunlu Gong, Liancheng Zhou, Qi Xia, Shan Chang, Jun Fang, Li Zhang   +5 more
doaj   +1 more source

Galactic Cosmic Rays Throughout the Heliosphere and in the Very Local Interstellar Medium. [PDF]

Space Sci Rev, 2022
Rankin JS, Bindi V, Bykov AM, Cummings AC, Della Torre S, Florinski V, Heber B, Potgieter MS, Stone EC, Zhang M.   +9 more
europepmc   +1 more source

Parkes Radio and NuSTAR X-Ray Observations of the Composite Supernova Remnant B0453–685 in the Large Magellanic Cloud

The Astrophysical Journal
Gamma-ray emission is observed coincident in position to the evolved, composite supernova remnant (SNR) B0453–685. Prior multiwavelength investigations of the region indicate that the pulsar wind nebula (PWN) within the SNR is the most likely origin for ...
Jordan Eagle, Jeremy Hare, Elizabeth Hays, Daniel Castro, Joseph Gelfand, Jwaher Alnaqbi, Matthew Kerr, Shi Dai, Jean Ballet, Fabio Acero, Patrick Slane, Marco Ajello   +11 more
doaj   +1 more source

PIC methods in astrophysics: simulations of relativistic jets and kinetic physics in astrophysical systems. [PDF]

Living Rev Comput Astrophys, 2021
Nishikawa K, Duţan I, Köhn C, Mizuno Y.   +3 more
europepmc   +1 more source

Variability of the Vela Pulsar Wind Nebula Observed with [ITAL]Chandra[/ITAL] [PDF]

, 2001
George G. Pavlov, Oleg Y. Kargaltsev, Divas Sanwal, Gordon P. Garmire, George G. Pavlov, Oleg Y. Kargaltsev, Divas Sanwal, Gordon P. Garmire   +7 more
openalex   +1 more source

Investigating the multiband non-thermal emission of the 100 TeV source eHWC J2019+368 with a pulsar wind nebula scenario [PDF]

, 2020
Jun Fang, Lu Wen, Huan Yu, S. Z. Chen
openalex   +1 more source

The Vela Pulsar and Its Pulsar Wind Nebula Vela-X Using 13 Yr of Fermi-LAT Observations

The Astrophysical Journal
We present results of more than 13 yr of Fermi–Large Area Telescope (LAT) data analysis for the Vela pulsar from 60 MeV to 100 GeV and its pulsar wind nebula (PWN), Vela X, for E  > 1 GeV in the off-pulse phases.
Alexander Lange, J. Eagle, O. Kargaltsev, Lucien Kuiper, Jeremy Hare   +4 more
doaj   +1 more source

HIGH-RESOLUTION X-RAY OBSERVATIONS OF THE PULSAR WIND NEBULA ASSOCIATED WITH THE GAMMA-RAY SOURCE HESS J1640–465 [PDF]

, 2009
A. Lemière, P. Slane, B. M. Gaensler, Sean Murray   +3 more
openalex   +1 more source