Results 81 to 90 of about 8,336 (234)

Non-detection of a pulsar-powered nebula in Puppis A, and implications for the nature of the radio-quiet neutron star RX J0822-4300 [PDF]

open access: yes, 2000
We report on a deep radio search for a pulsar wind nebula associated with the radio-quiet neutron star RX J0822-4300 in the supernova remnant Puppis A. The well-determined properties of Puppis A allow us to constrain the size of any nebula to less than ...
B. M. Gaensler   +9 more
core   +3 more sources

Solution to the sigma problem of pulsar wind nebulae [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society: Letters, 2013
Abstract We present first results of 3D relativistic magnetohydrodynamical simulations of pulsar wind nebulae. They show that the kink instability and magnetic dissipation inside these nebulae may be the key processes allowing them to reconcile their observations with the theory of pulsar winds. In particular, the size of the termination
Rony Keppens   +3 more
openaire   +4 more sources

Spatial Variations and Breaks in the Optical–Near-infrared Spectra of the Pulsar and Pulsar Wind Nebula in Supernova Remnant 0540–69.3

open access: yesThe Astrophysical Journal
The supernova remnant (SNR) 0540–69.3, twin of the Crab Nebula, offers an excellent opportunity to study the continuum emission from a young pulsar and pulsar wind nebula (PWN). We present observations taken with the Very Large Telescope instruments MUSE
L. Tenhu   +6 more
doaj   +1 more source

The G292.0+1.8 pulsar wind nebula in the mid-infrared

open access: yes, 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
core   +1 more source

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

GeV Gamma-Ray Emission from Pulsar Wind Nebula HESS J1356-645 with Fermi-Large Area Telescope

open access: yesThe Astrophysical Journal, 2023
HESS J1356-645 is considered to be a pulsar wind nebula (PWN) associated with the pulsar PSR J1357-6429. We reanalyze the GeV gamma-ray emission in the direction of HESS J1356-645 with more than 13 yr of Fermi-Large Area Telescope data.
Xi Liu   +4 more
doaj   +1 more source

A possible association of the new VHE gamma-ray source HESS J1825--137 with the pulsar wind nebula G18.0--0.7

open access: yes, 2005
We report on a possible association of the recently discovered very high-energy $\gamma$-ray source HESS J1825--137 with the pulsar wind nebula (commonly referred to as G 18.0--0.7) of the $2.1\times 10^{4}$ year old Vela-like pulsar PSR B1823--13.
A. Djannati-Ataï   +114 more
core   +2 more sources

G359.95-0.04: Pulsar Candidate Near Sgr A* [PDF]

open access: yes, 2005
We report the discovery of a prominent nonthermal X-ray feature located near the Galactic center that we identify as an energetic pulsar wind nebula. This feature, G359.95-0.04, lies 1 lyr north of Sgr A* (in projection), is comet-like in shape, and has ...
Gotthelf, E. V., Lu, F. J., Wang, Q. D.
core   +3 more sources

Gigahertz-peaked spectra pulsars in Pulsar Wind Nebulae [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2017
We have carried out a detailed study of the spectral nature of six pulsars surrounded by Pulsar wind nebulae (PWN). The pulsar flux density were estimated using the interferometric imaging technique of the Giant Metrewave Radio Telescope at three frequencies 325 MHz, 610 MHz and 1280 MHz. The spectra showed a turnover around gigahertz frequency in four
Karolina Rożko   +4 more
openaire   +3 more sources

Pulsar Wind Nebulae with Thick Toroidal Structure

open access: yes, 2011
We investigate a class of pulsar wind nebulae that show synchrotron emission from a thick toroidal structure. The best studied such object is the small radio and X-ray nebula around the Vela pulsar, which can be interpreted as the result of interaction ...
Abdo   +19 more
core   +1 more source

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