Pre-Supernova Shell Mergers: A New Source of Titanium-44?
Published:Dec 19, 2025 15:38
•1 min read
•ArXiv
Analysis
This article discusses a specific astrophysical phenomenon relevant to understanding the origins of elements. The research, published on ArXiv, is a highly technical discussion not broadly accessible to a general audience but important for experts in astrophysics.
Key Takeaways
- •The research investigates pre-supernova processes.
- •It focuses on the production of Titanium-44.
- •The findings suggest a potential new source of this element.
Reference
“Pre-supernova O-C shell mergers could produce more $^{44}\mathrm{Ti}$ than the explosion.”