Results 1 to 10 of about 54,876 (252)

Broadband X-Ray Spectroscopy of the Pulsar Wind Nebula in HESS J1640-465 [PDF]

open access: goldThe Astrophysical Journal, 2023
We present updated measurements of the X-ray properties of the pulsar wind nebula associated with the TeV γ -ray source HESS J1640-465 derived from Chandra and Nuclear Spectroscopic Telescope Array data.
Moaz Abdelmaguid   +3 more
doaj   +4 more sources

X-Ray Characterization of the Pulsar PSR J1849−0001 and Its Wind Nebula G32.64+0.53 Associated with TeV Sources Detected by H.E.S.S., HAWC, Tibet ASγ, and LHAASO

open access: greenThe Astrophysical Journal, 2023
We report on the X-ray emission properties of the pulsar PSR J1849−0001 and its wind nebula (PWN), as measured by Chandra, XMM-Newton, NICER, Swift, and NuSTAR.
Chanho Kim   +8 more
doaj   +4 more sources

Hard X-Ray Observation and Multiwavelength Study of the PeVatron Candidate Pulsar Wind Nebula “Dragonfly” [PDF]

open access: yesThe Astrophysical Journal, 2023
We studied the PeVatron nature of the pulsar wind nebula (PWN) G75.2+0.1 (“Dragonfly”) as part of our NuSTAR observational campaign of energetic PWNe. The Dragonfly is spatially coincident with LHAASO J2018+3651, whose maximum photon energy is 0.27 PeV ...
Jooyun Woo   +7 more
doaj   +2 more sources

A Spatially Resolved X-Ray Polarization Map of the Vela Pulsar Wind Nebula [PDF]

open access: yesThe Astrophysical Journal Letters, 2023
In this paper, we present a full spatially resolved polarization map for the Vela pulsar wind nebula (PWN) observed by IXPE. By employing effective background discrimination techniques, our results show a remarkably high degree of local polarization in ...
Kuan Liu   +14 more
doaj   +2 more sources

High-resolution Radio Study of the Dragonfly Pulsar Wind Nebula Powered by PSR J2021+3651 [PDF]

open access: yesThe Astrophysical Journal, 2023
The Dragonfly Nebula (G75.2+0.1) powered by the young pulsar J2021+3651 is a rare pulsar wind nebula (PWN) that shows double tori and polar jets enclosed by a bow-shock structure in X-rays.
Ruolan Jin   +3 more
doaj   +2 more sources

A Broadband X-Ray Study of the Rabbit Pulsar Wind Nebula Powered by PSR J1418-6058 [PDF]

open access: yesThe Astrophysical Journal, 2023
We report on broadband X-ray properties of the Rabbit pulsar wind nebula (PWN) associated with the pulsar PSR J1418−6058 using archival Chandra and XMM-Newton data, as well as a new NuSTAR observation.
Jaegeun Park   +6 more
doaj   +2 more sources

Discovery of GeV Gamma-Ray Emission from Pulsar Wind Nebula Kes 75 and PSR J1846–0258 [PDF]

open access: yesThe Astrophysical Journal, 2023
We report the detection of gamma-ray emission from pulsar wind nebula (PWN) Kes 75 and PSR J1846−0258. Through modeling the spectral energy distribution incorporating the new Fermi-LAT data, we find that the observed gamma-ray emission is likely a ...
Samayra M. Straal   +2 more
doaj   +2 more sources

A NuSTAR and Chandra Investigation of the Misaligned Outflow of PSR J1101–6101 and the Lighthouse Pulsar Wind Nebula [PDF]

open access: yesThe Astrophysical Journal, 2023
PSR J1101–6101 is an energetic young pulsar that powers the remarkable Lighthouse pulsar wind nebula (PWN). The pulsar belongs to the rare type of radio- and gamma-ray-quiet pulsars that are bright in hard X-rays.
Noel Klingler   +4 more
doaj   +2 more sources

Shedding new light on the Crab with polarized X-rays [PDF]

open access: yesScientific Reports, 2017
Strong magnetic fields, synchrotron emission, and Compton scattering are omnipresent in compact celestial X-ray sources. Emissions in the X-ray energy band are consequently expected to be linearly polarized. X-ray polarimetry provides a unique diagnostic
M. Chauvin   +15 more
doaj   +2 more sources

Testing a stochastic acceleration model of pulsar wind nebulae: early evolution of a wind nebula associated with SN 1986J [PDF]

open access: greenMonthly notices of the Royal Astronomical Society, 2023
Over three thousand pulsars have been discovered, but none have been confirmed to be younger than a few hundred years. Observing a pulsar after a supernova explosion will help us understand the properties of newborn ones, including their capability to ...
Shuta Tanaka, Kazumi Kashiyama
openalex   +3 more sources

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