Insights into the Properties of Type Ibn/Icn Supernovae and Their Progenitor Channels through X-Ray Emission

Type Ibn/Icn supernovae (SNe Ibn/Icn), which are characterized by narrow helium or carbon lines that originated in hydrogen-poor dense circumstellar medium (CSM), provide new insights into the final evolution of massive stars. While SNe Ibn/Icn are expected to emit strong X-rays through the strong s...

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Bibliographic Details
Published inThe Astrophysical journal Vol. 980; no. 1; pp. 86 - 99
Main Authors Inoue, Yusuke, Maeda, Keiichi
Format Journal Article
LanguageEnglish
Published The American Astronomical Society 10.02.2025
IOP Publishing
Subjects
Circumstellar matter
Stellar evolution
X-ray transient sources
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