Results 61 to 70 of about 706 (178)

Electromagnetic Signatures from Pulsar Remnants of Binary Neutron Star Mergers: Prospects for Unique Identification Using Multiwavelength Signatures

open access: yesThe Astrophysical Journal Letters
Binary neutron star (BNS) mergers can result in the formation of long-lived magnetar remnants that can enhance neutrino and electromagnetic (EM) emissions.
Mainak Mukhopadhyay, Shigeo S. Kimura
doaj   +1 more source

Possible Neutrino Emission from the Pulsar Wind Nebula G63.7+1.1

open access: yesThe Astrophysical Journal
We report on our finding of an excess of $5{4}_{-15}^{+16}$ neutrinos at the location of the pulsar wind nebula (PWN) G63.7+1.1. By analyzing the IceCube track-like neutrino data for a group of 14 PWNe, which are selected as targets because of their ...
Shunhao Ji   +3 more
doaj   +1 more source

Additional evidence for a pulsar wind nebula in SN 1987A from multi-epoch X-ray data and MHD modelling

open access: green, 2022
Emanuele Greco   +11 more
openalex   +2 more sources

Discovery of a Young, Highly Scattered Pulsar PSR J1032-5804 with the Australian Square Kilometre Array Pathfinder

open access: yesThe Astrophysical Journal
We report the discovery of a young, highly scattered pulsar in a search for highly circularly polarized radio sources as part of the Australian Square Kilometre Array Pathfinder Variables and Slow Transients survey.
Ziteng Wang   +9 more
doaj   +1 more source

Pulsar-wind-nebula-powered Galactic center X-ray filament G0.13-0.11: Proof of the synchrotron nature by IXPE [PDF]

open access: green, 2023
E. Churazov   +99 more
openalex   +1 more source

NuSTAR and XMM-Newton Observations of PSR J1930+1852 and Its Pulsar Wind Nebula

open access: yesThe Astrophysical Journal
Synchrotron X-ray emission from a pulsar wind nebula (PWN) is a sensitive probe of its magnetic field and high-energy particle population. Here we analyze contemporaneous NuSTAR and XMM - Newton observations of the PWN G54.1+0.3, powered by pulsar PSR ...
J. A. J. Alford   +2 more
doaj   +1 more source

Discovery of a radio emitting neutron star with an ultra-long spin period of 76 seconds. [PDF]

open access: yesNat Astron, 2022
Caleb M   +21 more
europepmc   +1 more source

X-Ray Polarization Detection of the Pulsar Wind Nebula in G21.5–0.9 with IXPE

open access: yesThe Astrophysical Journal
We present the X-ray polarization observation of G21.5−0.9, a young Galactic supernova remnant (SNR), conducted with the Imaging X-ray Polarimetry Explorer (IXPE) in 2023 October, with a total livetime of approximately 837 ks.
Niccolò Di Lalla   +100 more
doaj   +1 more source

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