Results 81 to 90 of about 6,070 (203)

Magnetoluminescence

, 2017
Pulsar Wind Nebulae, Blazars, Gamma Ray Bursts and Magnetars all contain regions where the electromagnetic energy density greatly exceeds the plasma energy density.
A. Hewish, A. Levinson, A. Rudy, A. Spitkovsky, A.A. Philippov, A.E. Broderick, A.P. Marscher, A.Y. Chen, B. Cerutti, B. Cerutti, B. Cerutti, B.L. Fanaroff, C. Kouveliotou, C. Thompson, C. Thompson, C.A. Wilson-Hodge, C.F. Kennel, D. Biskamp, D. Kagan, D. Lohse, D.A. Uzdensky, D.A. Uzdensky, D.L. Meier, D.R. Lorimer, E. Beltrami, E. Priest, E.N. Parker, F. Aharonian, F. Guo, F. Yuan, G. Madejski, G. Reber, G.R. Burbidge, G.R. Werner, H.K. Moffatt, H.K. Moffatt, H.P. Furth, I.F. Mirabel, J. Albert, J. Aleksić, J. Arons, J. Arons, J. Zrake, J.B. Taylor, J.B. Taylor, J.F. Drake, J.G. Kirk, J.J. Hester, J.J. Hester, K. Hurley, K. Hurley, K. Nalewajko, L. Sironi, L. Sironi, L. Sironi, L. Sironi, M. Ackermann, M. Hoshino, M. Hoshino, M. Hoshino, M. Lyutikov, M. Lyutikov, M. Schmidt, M.A. Belyaev, M.A. Riquelme, M.C. Begelman, M.C. Begelman, M.C. Weisskopf, M.J. Rees, M.J. Reid, M.N. Rosenbluth, M.P. Brenner, M.W. Kunz, P.G. Tait, P.M. Bellan, R. Blandford, R. Buehler, R. Giacconi, R.D. Blandford, R.D. Blandford, R.D. Blandford, R.W. Klebesadel, S. Chandrasekhar, S. Childress, S. Mereghetti, S. Zenitani, S.E. Boggs, S.I. Syrovatskii, S.S. Komissarov, S.S. Komissarov, S.S. Komissarov, T. Gold, T.W. Speiser, V. Arnol’d, V. Zhdankin, V.F. Hess, V.L. Fish, V.S. Imshennik, W. Horton, W. Max-Moerbeck, W.D. Evans, W.E. East, X. Wang, Y. Yuan, Y. Yuan   +104 more
core   +1 more source

Exploiting morphological data from Pulsar Wind Nebulae via a spatiotemporal leptonic transport code [PDF]

, 2020
Carlo van Rensburg, C. Venter, A. S. Seyffert, A. K. Harding   +3 more
openalex   +1 more source

Anticorrelation Between Flux and Photon Index of Hard-X-Ray Emission from the Crab

The Astrophysical Journal
Using Swift Burst Alert Telescope event-mode data during gamma-ray burst occurrences, we conduct spectral analysis for the Crab system. From 38 good observations, which span a period of 18 yr from 2006 to 2023, we find that the Crab’s X-ray flux not only
Koothodil Abhijith Augustine, Hsiang-Kuang Chang   +1 more
doaj   +1 more source

Future X-ray Polarimetry of Relativistic Accelerators: Pulsar Wind Nebulae and Supernova Remnants

Galaxies, 2018
Supernova remnants (SNRs) and pulsar wind nebulae (PWNs) are among the most significant sources of non-thermal X-rays in the sky, and the best means by which relativistic plasma dynamics and particle acceleration can be investigated.
Niccolò Bucciantini
doaj   +1 more source

Bow shocks around pulsars and neutron stars

, 2005
Pulsar wind nebulae are now well established as important probes both of neutron stars' relativistic winds and of the surrounding interstellar medium.
Aldcroft, Arzoumanian, Bryan M. Gaensler, Bucciantini, Bucciantini, Camilo, Caraveo, Chatterjee, Chatterjee, Chatterjee, Chen, Cordes, Gaensler, Gaensler, Gaensler, Gaensler, Gallant, Gvaramadze, Jones, Kaper, Kaspi, Mann, Moon, Ng, Olbert, Petre, Stappers, Sutherland, van Buren, van der Swaluw, van Kerkwijk, Wang, Wilkin, Wilkin, Zank, Zavlin   +35 more
core   +2 more sources

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

Potential Contribution of Young Pulsar Wind Nebulae to Galactic High-energy Neutrino Emission

The Astrophysical Journal
Pulsar wind nebulae (PWNe), especially the young ones, are among the most energetic astrophysical sources in the Galaxy. It is usually believed that the spin-down energy injected from the pulsars is converted into magnetic field and relativistic ...
Xuan-Han Liang, Xiao-Bin Chen, Ben Li, Ruo-Yu Liu, Xiang‐Yu Wang   +4 more
openalex   +2 more sources

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

LHAASO and Galactic cosmic rays. [PDF]

Innovation (Camb), 2022
Yang R.
europepmc   +1 more source

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