Uniform Distribution of the Extremely Overionized Plasma Associated with the Supernova Remnant G359.1-0.5
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab80ba/pdf
Reference61 articles.
1. Exploring a SNR/molecular cloud association within HESS J1745–303
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3. Deep X-Ray Observations of Supernova Remnants G359.1–0.5 and G359.0–0.9 with ASCA
4. ChandraACIS-I particle background: an analytical model
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1. Progenitor Constraint-incorporating Shell Merger: The Case of Supernova Remnant G359.0–0.9;The Astrophysical Journal;2024-07-01
2. On the Formation of Over-ionized Plasma in Evolved Supernova Remnants;The Astrophysical Journal;2022-10-01
3. Spatially resolved study of the SS 433/W 50 west region with Chandra: X-ray structure and spectral variation of non-thermal emission;Publications of the Astronomical Society of Japan;2022-08-11
4. Spatially Decomposed γ-Ray Features Surrounding Supernova Remnant Kes 79 and PSR J1853+0056;The Astrophysical Journal;2022-03-01
5. Spatially resolved X-ray study of the mixed morphology SNR G359.1-0.5;Monthly Notices of the Royal Astronomical Society;2022-02-23
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