Results 121 to 130 of about 11,249 (249)

HESS Observations of Pulsar Wind Nebulae [PDF]

open access: yesAIP Conference Proceedings, 2005
6 pages, 3 figures, appeared in the proceedings of "Astrophysical Sources of High Energy Particles and Radiation", held in Torun, Poland, eds. T. Bulik, B.
openaire   +3 more sources

Precise Measurements of TeV Halos around Geminga and Monogem Pulsars with HAWC

open access: yesThe Astrophysical Journal
We present the most precise measurements to date for the spatial extension and energy spectrum of the γ -ray region between a pulsar’s wind nebula and the interstellar medium, better known as the halo, present around Geminga and PSR B0656+14 (Monogem ...
A. Albert   +94 more
doaj   +1 more source

Positrons from pulsar winds

open access: yes, 2010
Pulsars, or more generally rotation powered neutron stars, are excellent factories of antimatter in the Galaxy, in the form of pairs of electrons and positrons.
Amato, Elena, Blasi, Pasquale
core   +1 more source

The Devil is in the Details: Compact Structures in Pulsar Wind Nebulae

open access: yes, 2005
The large-scale structure of pulsar wind nebulae (PWNe) tells us a considerable amount about their average magnetic fields, the total particle input from the pulsar winds, and the confining pressure at their outer boundaries.
Aschenbach   +36 more
core   +2 more sources

Pulsar wind nebulae in supernova remnants

open access: yesAstronomy and Astrophysics, 2000
10 pages, 9 figures, submitted to Astronomy and ...
van der Swaluw, E.   +3 more
openaire   +3 more sources

Gamma-rays from the Pulsar Wind Nebulae [PDF]

open access: yesAIP Conference Proceedings, 2003
15 pages, 11 figures, A&A style, will be published in A& ...
M. Bartosik, W. Bednarek
openaire   +5 more sources

An X-Ray Synchrotron Shell and a Pulsar: The Peculiar Supernova Remnant G32.4+0.1

open access: yesThe Astrophysical Journal
We present a deep Chandra observation of the shell supernova remnant (SNR) G32.4+0.1, whose featureless X-ray spectrum has led to its classification as an X-ray synchrotron-dominated SNR. We find a partial shell morphology whose outline is quite circular,
Stephen P. Reynolds   +1 more
doaj   +1 more source

Turbulent Transport Characteristics of the Particles within Pulsar Wind Nebulae 3C58 and G54.1+0.3

open access: yesThe Astrophysical Journal
Turbulent transport characteristics of the particles within two Crab-like pulsar wind nebulae (PWNe), 3C58 and G54.1+0.3, are investigated in the framework of a time-dependent turbulent diffusion model.
Fang-Wu Lu, Bo-Tao Zhu, Wen Hu, Li Zhang
doaj   +1 more source

Resolving the Crab pulsar wind nebula at teraelectronvolt energies [PDF]

open access: yesNature Astronomy, 2019
23 pages, 5 ...
A. Dmytriiev   +206 more
openaire   +13 more sources

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

open access: yesGalaxies, 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

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