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...
Guardado en:
| Autores principales: | , , , , , , , , |
|---|---|
| Formato: | Artigo |
| Lenguaje: | Inglês |
| Publicado: |
EDP Sciences
2026-05-01
|
| Colección: | Astronomy & Astrophysics |
| Materias: | |
| Acceso en línea: | https://www.aanda.org/articles/aa/full_html/2026/05/aa56500-25/aa56500-25.html |
| Etiquetas: |
Sin Etiquetas, Sea el primero en etiquetar este registro!
|