Results 11 to 20 of about 8,188 (190)
The imprint of pulsar parameters on the morphology of Pulsar Wind Nebulae [PDF]
Monthly Notices of the Royal Astronomical Society, 2016 Monthly notices of the Royal Astronomical Society 462(3), 2762 - 2776 (2016).
Bühler, Rolf, Giomi, Matteo
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Pulsar wind nebulae in supernova remnants [PDF]
Astronomy and Astrophysics, 2000 10 pages, 9 figures, submitted to Astronomy and ...
van der Swaluw, E. +3 more
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DA 495: An Aging Pulsar Wind Nebula [PDF]
The Astrophysical Journal, 2008 We present a radio continuum study of the pulsar wind nebula (PWN) DA 495 (G65.7+1.2), including images of total intensity and linear polarization from 408 to 10550 MHz based on the Canadian Galactic Plane Survey and observations with the Effelsberg 100-m Radio Telescope.
Roland Kothes +5 more
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Optical identification of the 3C 58 pulsar wind nebula [PDF]
, 2008 We have performed a deep optical imaging of 3C 58 SNR with the NOT in the B and V bands to detect the optical counterpart of the associated pulsar J0295+6449 and its torus-like wind nebula visible in X-rays.
Yu. A. Shibanov +4 more
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The Supernova Remnant G106.3+2.7 and Its Pulsar‐Wind Nebula: Relics of Triggered Star Formation in a Complex Environment [PDF]
, 2001 We propose that the pulsar nebula associated with the pulsar J2229+6114 and the supernova remnant (SNR) G106.3+2.7 are the result of the same supernova explosion.
R. Kothes +2 more
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ChandraConfirmation of a Pulsar Wind Nebula in DA 495 [PDF]
, 2008 As part of a multiwavelength study of the unusual radio supernova remnant DA 495, we present observations made with the Chandra X-ray Observatory. Imaging and spectroscopic analysis confirms the previously detected X-ray source at the heart of the ...
Zaven Arzoumanian +4 more
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The Theory of Pulsar Winds and Nebulae [PDF]
, 2009 We review current theoretical ideas on pulsar winds and their surrounding nebulae. Relativistic MHD models of the wind of the aligned rotator, and of the striped wind, together with models of magnetic dissipation are discussed. It is shown that the observational signature of this dissipation is likely to be point-like, rather than extended, and that ...
John G. Kirk +2 more
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Supernova remnants in nearby galaxies
Astronomische Nachrichten, Volume 341, Issue 2, Page 156-162, February 2020., 2020 Abstract Supernova remnants (SNRs) are the aftermath of stellar explosions, which inject large amounts of energy into the interstellar medium (ISM), carving out new structures and transferring kinetic energy to the ISM. They also act as recycling centers, which return elements processed in stars to the ISM, and cosmic particle accelerators.
Manami Sasaki
wiley +1 more source
Magnetic Reconnection in the Space Sciences: Past, Present, and Future
Journal of Geophysical Research: Space Physics, Volume 125, Issue 2, February 2020., 2020 Abstract Magnetic reconnection converts, often explosively, stored magnetic energy to particle energy in space and in the laboratory. Through processes operating on length scales that are tiny, it facilitates energy conversion over dimensions of, in some cases, hundreds of Earth radii.
M. Hesse, P. A. Cassak
wiley +1 more source
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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