Uncovering Magnetic Turbulence in Young Supernova Remnants with Polarized X-Ray Imaging
Author:
Funder
NASA
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/aba960/pdf
Reference67 articles.
1. Cosmic Radiation and Radio Stars
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5. The Acceleration of Galactic Cosmic Rays
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1. X-ray polarization: A view deep inside cosmic ray driven turbulence and particle acceleration in supernova remnants;Physical Review D;2024-07-30
2. Discovery of a Shock-compressed Magnetic Field in the Northwestern Rim of the Young Supernova Remnant RX J1713.7–3946 with X-Ray Polarimetry;The Astrophysical Journal Letters;2024-05-30
3. Nonthermal Processes and Particle Acceleration in Supernova Remnants;Handbook of X-ray and Gamma-ray Astrophysics;2024
4. Turbulent Structure in Supernova Remnants G46.8−0.3 and G39.2−0.3 from THOR Polarimetry;The Astrophysical Journal;2023-10-30
5. Magnetic Structures and Turbulence in SN 1006 Revealed with Imaging X-Ray Polarimetry;The Astrophysical Journal;2023-10-27
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