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Acceleration and Transport of the Unstable Cosmic-Ray Isotope 60Fe in Supernova-enriched Environments

The unstable isotope ^60 Fe, with a half-life of 2.6 million years, is produced primarily in supernova explosions. The observed presence of ^60 Fe in cosmic rays and its detection in deep-sea crusts and sediments suggest two possible scenarios: either the direct acceleration of ^60 Fe from supernova...

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Bibliografski detalji
Glavni autori: Xin-Yue Shi, Martin Pohl, Michael M. Schulreich
Format: Artigo
Jezik:Inglês
Izdano: IOP Publishing 2025-01-01
Serija:The Astrophysical Journal
Teme:
Online pristup:https://doi.org/10.3847/1538-4357/adea4c
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