Results 61 to 70 of about 54,876 (252)
Pulsar Wind Nebulae in the SKA era [PDF]
Proceedings of Advancing Astrophysics with the Square Kilometre Array — PoS(AASKA14), 2015 Comments: 10 pages, 3 figures, to be published in: "Advancing Astrophysics with the Square Kilometre Array", Proceedings of Science, PoS(AASKA14)
Roberts, MSE +6 more
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The Polarized Cosmic Hand: IXPE Observations of PSR B1509−58/MSH 15−52
The Astrophysical Journal, 2023 We describe IXPE polarization observations of the pulsar wind nebula (PWN) MSH 15−5 ^2 , the “Cosmic Hand.” We find X-ray polarization across the PWN, with B -field vectors generally aligned with filamentary X-ray structures.
Roger W. Romani +102 more
doaj +1 more source
Universe, 2023 Based on the expected population of core collapse supernova remnants and the huge number of detected pulsars in the Galaxy, still representing only a fraction of the real population, pulsar wind nebulae are likely to constitute one of the largest classes of extended Galactic sources in many energy bands. For simple evolutionary reasons, the majority of
openaire +3 more sources
Prospects for observations of pulsars and pulsar wind nebulae with CTA [PDF]
Astroparticle Physics, 2013 accepted for publication in Astroparticle ...
E. d. Ona Wilhelmi +18 more
openaire +4 more sources
The Astrophysical Journal, 2023 Motivated by the recent discovery of a low-surface-brightness diffuse emission, a supernova remnant (SNR) candidate, surrounding the young pulsar PSR J0837–2454, we carry out a likelihood analysis of the γ -ray data obtained by the Fermi Gamma-ray Space ...
Pengfei Zhang, Yuliang Xin
doaj +1 more source
The braking index of PSR B0540−69 and the associated pulsar wind nebula emission after spin-down rate transition [PDF]
Monthly notices of the Royal Astronomical Society, 2020 In 2011 December, PSR B054−69 experienced a spin-down rate transition (SRT), after which the spin-down power of the pulsar increased by $\sim 36{{\ \rm per\ cent}}$. About 1000 d after the SRT, the X-ray luminosity of the associated pulsar wind nebula (
L. Wang +8 more
semanticscholar +1 more source
A deep search for pulsar wind nebulae using pulsar gating [PDF]
Monthly Notices of the Royal Astronomical Society, 1999 10 pages, 5 figures, MNRAS in ...
Ben Stappers +4 more
openaire +7 more sources
THE THEORY OF PULSAR WIND NEBULAE [PDF]
International Journal of Modern Physics: Conference Series, 2014 I will review the current status of our theoretical understanding of Pulsar Winds and associated nebulae (PWNe). In recent years, axisymmetric models of pulsar winds with a latitude dependent energy flux have proved very successful at explaining the morphology of PWNe as seen in the X-rays.
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Interaction of a magnetized pulsar wind with its surroundings. MHD simulations of Pulsar Wind Nebulae [PDF]
Astron.Astrophys. 404 (2003) 939-948, 2003 Magnetohydrodynamical simulations are presented of a magnetized pulsar wind interacting directly with the interstellar medium, or, in the case of a surrounding supernova remnant, with the associated freely expanding ejecta of the progenitor star. In both cases the simulations show that the pulsar wind nebula will be elongated due to the dynamical ...
arxiv +1 more source
PULSAR WIND NEBULAE MODELING [PDF]
International Journal of Modern Physics: Conference Series, 2014 Pulsar Wind Nebulae (PWNe) are ideal astrophysical laboratories where high energy relativistic phenomena can be investigated. They are close, well resolved in our observations, and the knowledge derived in their study has a strong impact in many other fields, from AGNs to GRBs.
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