NuSTAR and Chandra Observations of the Galactic Center Nonthermal X-Ray Filament G0.13–0.11: A Pulsar-wind-nebula-driven Magnetic Filament

NuSTAR and Chandra Observations of the Galactic Center Nonthermal X-Ray Filament G0.13–0.11: A Pulsar-wind-nebula-driven Magnetic Filament

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© 2020. The American Astronomical Society. All rights reserved. One of the most unique phenomena in the Galactic center region is the existence of numerous long and narrow filamentary structures within a few hundred parsecs of Sgr A∗. While more than 100 radio filaments have been revealed by MeerKAT...

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Bibliographic Details
Main Authors: Zhang, Shuo, Zhu, Zhenlin, Li, Hui, Pasham, Dheeraj, Li, Zhiyuan, Clavel, Maïca, Baganoff, Frederick K, Perez, Kerstin, Mori, Kaya, Hailey, Charles J
Format: Article
Language:English
Published: American Astronomical Society 2021
Online Access:https://hdl.handle.net/1721.1/132365

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https://hdl.handle.net/1721.1/132365

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