Results 81 to 90 of about 5,865 (191)

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
Basu, Rahul   +3 more
openaire   +2 more sources

4FGL J1844.4–0306: High-energy Emission Likely from the Supernova Remnant G29.37 + 0.1

open access: yesThe Astrophysical Journal, 2023
Very-high-energy (VHE) observations have revealed approximately 100 TeV sources in our Galaxy, and a significant fraction of them are under investigation to understand their origin. We report our study of one of them, HESS J1844−030.
Dong Zheng   +4 more
doaj   +1 more source

Understanding Pulsar Wind Nebulae with the SKA

open access: yesThe Open Journal of Astrophysics
Produced by the interaction between the "pulsar wind'' powered by the rotational energy of a neutron star and its surroundings, the study of pulsar wind nebulae (PWNe) provides vital insight into the physics of neutron star magnetospheres and ultra ...
Joseph D. Gelfand   +12 more
doaj   +1 more source

A deep search for pulsar wind nebulae using pulsar gating [PDF]

open access: yes, 1999
Using the Australia Telescope Compact Array (ATCA) we have imaged the fields around five promising pulsar candidates to search for radio pulsar wind nebulae (PWNe).
Gaensler, B. M.   +2 more
core   +2 more sources

MHD Interaction of Pulsar Wind Nebulae with SNRs and the ISM

open access: yes, 2005
In the late 1960s the discovery of the Crab pulsar in its associated supernova remnant, launched a new field in supernova remnant research: the study of pulsar-driven or plerionic supernova remnants.
Arzoumanian   +28 more
core   +2 more sources

Pulsar Wind Nebula candidates recently discovered by H.E.S.S. [PDF]

open access: yesAIP Conference Proceedings, 2008
4 pages, 6 figures, Submitted to Proceedings of "4th Heidelberg International Symposium on High Energy Gamma-Ray Astronomy 2008"
M. Renaud   +8 more
openaire   +4 more sources

Comparison between the Emission Torus and the Measured Toroidal Magnetic Field for the Crab and Vela Nebulae

open access: yesThe Astrophysical Journal
Polarization measurements provide insight into the magnetic field, a critical aspect of the dynamics and emission properties around the compact object.
Wei Deng   +7 more
doaj   +1 more source

INTEGRAL observations of TeV plerions

open access: yes, 2006
Amongst the sources seen in very high gamma-rays several are associated with Pulsar Wind Nebulae (``TeV plerions''). The study of hard X-ray/soft gamma-ray emission is providing an important insight into the energetic particle population present in these
A. Achterberg   +21 more
core   +1 more source

First Detection of Polarization in X-Rays for PSR B0540-69 and Its Nebula

open access: yesThe Astrophysical Journal
We report on X-ray polarization measurements of the extragalactic Crab-like PSR B0540-69 and its Pulsar Wind Nebula (PWN) in the Large Magellanic Cloud, using a ∼850 ks Imaging X-ray Polarimetry Explorer (IXPE) exposure. The PWN is unresolved by IXPE. No
Fei Xie   +103 more
doaj   +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

Home - About - Disclaimer - Privacy