Results 71 to 80 of about 8,830 (213)
X-Ray Spectroscopy of the Highly Magnetized Pulsar PSR J1846-0258, Its Wind Nebula, and Hosting Supernova Remnant Kes 75 [PDF]
, 2021 E. V. Gotthelf +3 more
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The G292.0+1.8 pulsar wind nebula in the mid-infrared
, 2009 G292.0+1.8 is a Cas A-like supernova remnant that contains the young pulsar PSR J1124-5916 powering a compact torus-like pulsar wind nebula visible in X-rays. A likely counterpart to the nebula has been detected in the optical VRI bands.
A. A. Danilenko +22 more
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The Pulsar Wind Nebula in G11.2−0.3
The Astrophysical Journal, 2003 We present an X-ray and radio study of the wind nebula surrounding the central pulsar PSR J1811-1925 in the supernova remnant G11.2-0.3. Using high resolution data obtained with the Chandra X-ray observatory and with the VLA radio telescope we show the X-ray and radio emission is asymmetric around the pulsar, despite the latter's central position in ...
Roberts, M. S. E. +7 more
openaire +2 more sources
PeV Emission of the Crab Nebula: Constraints on the Proton Content in Pulsar Wind and Implications [PDF]
, 2021 Ruo-Yu Liu, Xiang‐Yu Wang
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Polarization in Pulsar Wind Nebulae
, 2009 6 pages, 2 figures, workshop: Polarimetry days in Rome: Crab status, theory and prospects, October 16-17 2008, Rome ...
Volpi, D. +3 more
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Hard diffuse X-ray emission around the PSR\,J2032+4127: A pulsar wind nebula in the Cygnus\,OB2 association [PDF]
, 2020 Albacete Colombo J. F. +3 more
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Pulsar-wind nebulae in X-rays and TeV gamma-rays
, 2010 Pulsars are known to be efficient accelerators that produce copious amounts of relativistic particles and inject them into the Galactic medium. The radiation emitted by such a pulsar wind can be seen from radio through gamma-rays as a pulsar-wind nebula (
Kargaltsev, Oleg, Pavlov, George
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Optical observations of PSR J2021+3651 in the Dragonfly Nebula with the GTC
, 2015 PSR J2021+3651 is a 17 kyr old rotation powered pulsar detected in the radio, X-rays, and $\gamma$-rays. It powers a torus-like pulsar wind nebula with jets, dubbed the Dragonfly, which is very similar to that of the Vela pulsar.
Cabrera-Lavers, Antonio +9 more
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Three Concurrent Phases of Massive-Star Evolution in a Pulsar-Wind Nebula [PDF]
, 2010 The nebular material associated the the SNR G54.1+0.3 (hereafter G54) contains the the first reported instance of triggered star formation in the immediate vicinity of a Pulsar and its Wind Nebula (PWN). With 2MASS and Spitzer colors and followup near-IR
Hillier, D. John +4 more
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