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Inferring a Dense Confined Circumstellar Medium around Supernova Progenitors via Long-term Hydrodynamical Evolution

Circumstellar interaction of supernova (SN) ejecta is an essential process in its evolution, and observations of SNe have found the signature of circumstellar interaction in both the early and late evolutionary phases of SNe. In this Letter, we show that if the SN forward shock plunges into a tenuou...

Disgrifiad llawn

Wedi'i Gadw mewn:
Manylion Llyfryddiaeth
Prif Awduron: Tomoki Matsuoka, Keiichi Maeda, Ke-Jung Chen
Fformat: Artigo
Iaith:Inglês
Cyhoeddwyd: IOP Publishing 2025-01-01
Cyfres:The Astrophysical Journal Letters
Pynciau:
Mynediad Ar-lein:https://doi.org/10.3847/2041-8213/adef08
Tagiau: Ychwanegu Tag
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