Confined Circumstellar Material as a Dust Formation Site in Type II Supernovae

We propose a model for dust formation in Type II supernovae (SNe) interacting with confined circumstellar material (CSM), motivated by recent time-domain surveys that have revealed a substantial fraction of SN progenitors to be surrounded by CSM ejected shortly before core collapse. We simulate the...

Full description

Bibliographic Details
Published in:The Astrophysical Journal
Main Authors: Yuki Takei, Kunihito Ioka, Masaru Shibata
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Subjects:
Supernovae
Circumstellar matter
Stellar mass loss
Interstellar dust
Online Access:https://doi.org/10.3847/1538-4357/ae0466

Internet

https://doi.org/10.3847/1538-4357/ae0466

Similar Items