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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Detalhes bibliográficos

Principais autores:	Chi Yi-Heng, Zhou Ping, Chen Yang, Sun Lei, Li Chengkui, Jia Shumei, Chen Yong, Ge Chong, Yuan Weimin
Formato:	Artigo
Idioma:	Inglês
Publicado em:	EDP Sciences 2026-05-01
Colecção:	Astronomy & Astrophysics
Assuntos:	plasmas ism: supernova remnants x-rays: ism
Acesso em linha:	https://www.aanda.org/articles/aa/full_html/2026/05/aa56500-25/aa56500-25.html
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