A complete X-ray view of supernova remnant W28 with the Einstein Probe: Spatial distribution of parameters, and the origin of the thermal-composite morphology
The question about what causes a supernova remnant (SNR) to be a thermal composite rather than have a typical shell-like morphology remains unsolved, as does what causes the plasma inside it to recombine. With the 13-ks observation of the Following-up X-ray Telescope on board the Einstein Probe, we...
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| Huvudupphov: | , , , , , , , , |
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| Materialtyp: | Artigo |
| Språk: | Inglês |
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EDP Sciences
2026-05-01
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| Serie: | Astronomy & Astrophysics |
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| Länkar: | https://www.aanda.org/articles/aa/full_html/2026/05/aa56500-25/aa56500-25.html |
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