Results 111 to 120 of about 1,321 (200)

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

The population point of view on the evolution of TeV pulsar wind nebulae [PDF]

, 2017
International audienceTo investigate the nature and evolution of TeV pulsar wind nebulae, we examine the firmly identified PWNe in the H.E.S.S. Galactic Plane Survey, along with the few other known detections from the literature, as well as the upper ...
H.E.S.S. Collaboration, Michael Mayer, Stefan Klepser, Klepser, Stefan, Valerius, Kathrin, Yves Gallant, Mayer, Michael, Kathrin Valerius, Gallant, Yves, Gallant, Yves A.   +9 more
core   +2 more sources

VHE,gamma-ray emitting pulsar wind nebulae discovered by HESS [PDF]

, 2007
Recent advances in very-high-energy (VHE) gamma-ray astronomy have opened a new observational window on the physics of pulsars. The high sensitivity of current imaging atmospheric Cherenkov telescopes, and in particular of the H.E.S.S. array, has already
Carrigan, S., Funk, S., Khelifi, B., Komin, Nukri, Hinton, J. A., Kosack, K., Komin, Nu., Gallant, Yves, Hoppe, S., Djannati-Atai, A., Masterson, C., Gallant, Y. A., Lemiere, A., de Jager, O. C.   +13 more
core   +2 more sources

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

The emerging population of pulsar wind nebulae in hard X-rays [PDF]

, 2008
Proceedings of the 2nd Simbol-X Symposium, AIP Conf. Proc. Series, Eds. P. Ferrando and J. Rodriguez (4 pages, 2 figures)International audienceThe hard X-ray synchrotron emission from pulsar wind nebulae (PWNe) probes energetic particles, closely related
Terrier, R., Falanga, M., Mattana, F., Renaud, M., Götz, D.   +4 more
core  

Full-3D relativistic MHD simulations of bow shock pulsar wind nebulae: dynamics [PDF]

, 2019
Bow shock pulsar wind nebulae (BSPWNe) are known to show a large variety of shapes and morphologies, both when comparing different objects, and for the same object in different energy bands.
Olmi, Barbara, BUCCIANTINI, NICCOLO'
core   +1 more source

Extreme Electron Acceleration with Fixed Radiation Energy. [PDF]

Entropy (Basel), 2022
Good MRR, Singha C, Zarikas V.
europepmc   +1 more source

Spatially Resolved Polarization Variation of the Crab Nebula

The Astrophysical Journal
We examined the spatially resolved polarization variations in the Crab Nebula over 2 yr, using observational data from the Imaging X-ray Polarimetry Explorer, and offer key insights into its magnetic field structures and evolution.
Chao Zuo, Fei Xie, Mingyu Ge, Wei Deng, Kuan Liu, Fabio La Monaca, Alessandro Di Marco, Wenhao Wei, Wei Chen   +8 more
doaj   +1 more source

The IXPE Science of Pulsars and Their Nebulae

Galaxies
Pulsars (PSRs) and Pulsar Wind Nebulae (PWNe) form some of the most interesting high-energy astrophysical systems. Their prominent synchrotron emission makes them ideal candidates for polarimetry.
Niccolò Bucciantini, Roger W. Romani, Fei Xie, Josephine Wong   +3 more
doaj   +1 more source

Veritas observations of Pulsar Wind Nebulae in the VHE band [PDF]

, 2010
Pulsars have been known to exist for over forty years now, but the nature of their emission throughout the EM spectrum is still not well understood.
Zitzer, Benjamin J
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