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

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. In the X-ray data, we detected the 38 ms pulsations of the pulsar up to ∼60 keV with high significance. Additionally, we found that the pul...

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Bibliographic Details

Published in:	The Astrophysical Journal
Main Authors:	Chanho Kim, Jaegeun Park, Jooyun Woo, Sarah Silverman, Hongjun An, Aya Bamba, Kaya Mori, Stephen P. Reynolds, Samar Safi-Harb
Format:	Article
Language:	English
Published:	IOP Publishing 2023-01-01
Subjects:	Pulsars Pulsar wind nebulae Rotation powered pulsars High energy astrophysics Gamma-ray sources X-ray sources
Online Access:	https://doi.org/10.3847/1538-4357/ad0ecd