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Double-degenerate Carbon–Oxygen and Oxygen–Neon White Dwarf Mergers: A New Mechanism for Faint and Rapid Type Ia Supernovae
Type Ia supernovae (SNe Ia) originate from the thermonuclear explosion of carbon–oxygen white dwarfs (CO WDs), giving rise to luminous optical transients. A relatively common variety of subluminous SNe Ia events, referred to as SNe Iax, are believed to arise from the failed detonation of a CO WD. In...
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| Publié dans: | Astrophys J |
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| Auteurs principaux: | , , , , |
| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
2018
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| Sujets: | |
| Accès en ligne: | https://ncbi.nlm.nih.gov/pmc/articles/PMC6350549/ https://ncbi.nlm.nih.gov/pubmed/30713344 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.3847/1538-4357/aaedb7 |
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