Wakes from Companion Interactions in Type Ia Supernovae Nebular Emission Line Profiles
Thermonuclear supernovae (SNe) are the result of the nuclear transformation of carbon/oxygen white dwarfs (WDs) to the radioactive element ^56 Ni and intermediate mass elements like Ca, Ar, etc. Most progenitor scenarios involve a companion star that donates matter to the exploding WD, implying a fu...
שמור ב:
| Principais autores: | , , |
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| פורמט: | Artigo |
| שפה: | Inglês |
| יצא לאור: |
IOP Publishing
2025-01-01
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| סדרה: | The Astrophysical Journal |
| נושאים: | |
| גישה מקוונת: | https://doi.org/10.3847/1538-4357/ae0734 |
| תגים: |
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