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Three-dimensional Structure of Incomplete Carbon–Oxygen Detonations in Type Ia Supernovae

Carbon–oxygen (CO) detonation with reactions terminating either after burning of ^12 C in the leading ^12 C +  ^12 C reaction or after burning of ^12 C and ^16 O to Si-group elements may occur in the low-density outer layers of exploding white dwarfs and be responsible for the production of intermed...

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Bibliografische Detailangaben
Hauptverfasser: A. Khokhlov, I. Domínguez, A. Y. Chtchelkanova, P. Hoeflich, E. Baron, K. Krisciunas, M. Phillips, N. Suntzeff, L. Wang
Format: Artigo
Sprache:Inglês
Veröffentlicht: IOP Publishing 2025-01-01
Schriftenreihe:The Astrophysical Journal
Schlagworte:
Online-Zugang:https://doi.org/10.3847/1538-4357/adb0c1
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